The galaxy presents as an elliptical morphology, exhibiting a smooth, relatively featureless light distribution. The core region displays a concentrated luminosity, appearing golden or yellow in color, suggestive of an older stellar population. There is a gradual decrease in light intensity moving outwards from the core towards the galaxy's edge. The outer regions of the galaxy show a bluer hue, hinting at the presence of a younger, although potentially sparse, stellar population. Overall the galaxy appears quite round. There is no evidence of significant disk structures, spiral arms, or ongoing major merger events. Faint wisps or disturbances can be observed, but they are not significantly noticeable and may be suggestive of a minor interaction or internal activity. 
