The galaxy appears to be elliptical in shape, exhibiting a smooth, featureless morphology. The light distribution is concentrated towards the center, suggesting a prominent bulge. The color profile indicates a redder hue, possibly indicative of an older stellar population and a lower rate of ongoing star formation within the galaxy. There is no evidence of spiral arms, a disk structure, or any significant tidal disturbances or merging activity. The overall appearance suggests a galaxy that is relatively relaxed and has likely undergone significant dynamical evolution.
