The galaxy presents a largely smooth, elliptical morphology. There is a highly concentrated, bright central region suggestive of a prominent galactic nucleus. The light distribution appears quite symmetrical, with a rapid falloff in brightness moving outward from the center. Color gradients are subtle, but the central region may exhibit a slightly bluer hue, potentially indicating a region of ongoing, albeit subdued, star formation activity. The outer regions appear redder, consistent with an older stellar population. No prominent spiral arms or distinct features of active star formation, such as HII regions, are discernible within the galaxy's structure. Overall, the galaxy exhibits characteristics consistent with a relatively quiescent and evolved system.
