The galaxy presents as a generally smooth, elliptical-like structure with a concentrated, bright central bulge. The color profile suggests a relatively older stellar population, evident in the redder hues concentrated within the core and inner regions. Fainter, slightly bluer light extends outwards from the central region suggesting some level of ongoing, but likely low, star formation within a small region of the galactic disc. Overall, it appears relatively undisturbed, exhibiting no strong signs of tidal interactions or major mergers. It does not look very active, and does not show strong signs of a spiral structure. The galaxy appears moderately massive.
