The galaxy presents as a relatively smooth, disk-like structure. The overall morphology appears to be an intermediate type, exhibiting characteristics between a pure elliptical and a spiral galaxy.

The galaxy exhibits a prominent central bulge that is concentrated. The central bulge appears to be surrounded by a flattened disk component. The disk is somewhat featureless, lacking any obvious spiral arm structures. The outer regions of the disk gradually fade into the background, suggesting a relatively smooth stellar density profile.

The color profile of the galaxy suggests a mix of stellar populations. The central bulge appears slightly redder in color than the disk, which implies a higher concentration of older, redder stars in the nucleus. The disk displays bluer hues, indicating the presence of younger, hotter stars and perhaps some ongoing star formation, albeit at a low rate. There are no significant dust lanes visible across the face of the galaxy. The overall light distribution suggests that it is not currently undergoing any major merging events or experiencing significant tidal disturbances.
