The galaxy presents as a somewhat elliptical, smooth object with a concentrated central bulge. The light distribution indicates a relatively even intensity gradient, gradually decreasing from the core outwards. The core appears yellowish, indicating the presence of an older stellar population. The surrounding disk exhibits a bluer hue, suggestive of more recent star formation activity. There is some indication of a faint, diffuse halo surrounding the main body of the galaxy. No distinct spiral arms are readily apparent, nor are there any obvious signs of ongoing major mergers or tidal disturbances.
