This galaxy presents as a fairly smooth, elliptical-like structure. It exhibits a concentrated central bulge with a gradual decrease in luminosity extending outwards. The galaxy appears to have a slight elongation, deviating from a perfectly circular shape. The color profile indicates a relatively redder hue overall, suggestive of an older stellar population. There is some hint of a faint disk component. No prominent spiral arms or significant dust lanes are apparent. The galaxy does not appear to be undergoing any major merging or tidal interactions.
