The galaxy presents as a somewhat elliptical, diffuse structure. The light distribution appears relatively smooth, with a concentrated central bulge that gradually fades into the outer regions of the galaxy. There is no distinct spiral arm structure apparent in this image, nor are there any signs of strong tidal features or morphological disturbances, such as those arising from a major merger.

The color profile indicates a dominance of older stellar populations, judging from the yellowish hue. The galaxy's overall appearance suggests a system that is relatively quiescent in terms of star formation. The shape is closer to in between round and cigar shaped. There is a high likelihood that the object is not currently undergoing major merging activity.
