The galaxy presents as a relatively smooth, elliptical-like structure. The central bulge is luminous, with a concentrated bright yellow-white hue, suggesting an older stellar population. The light diminishes gradually towards the outer regions, which appear fuzzier and less defined. There is little evidence of spiral arm structure or distinct dust lanes. Overall, it appears to be a galaxy dominated by an older, evolved stellar population and exhibiting limited ongoing star formation. It shows a regular and rounded morphology, without noticeable signs of significant tidal disturbances or mergers.
