The galaxy presents as a relatively smooth, elliptical-like object, characterized by a concentrated central bulge. It exhibits a yellowish-white color profile in the inner regions, suggestive of an older stellar population and minimal ongoing star formation. The outer edges show a slight decrease in surface brightness and shift towards a redder hue, likely indicating a further decrease in star formation activity and the presence of a predominantly older, redder stellar population in these regions. The overall shape is elongated, with a ratio of major to minor axis greater than 2, hinting at an E4-E6 morphological type. There are no readily apparent signs of spiral arms or significant dust lanes. No obvious tidal features or merging companions are observed.
