The galaxy presents as a relatively smooth, elliptical-like structure, exhibiting a concentrated central bulge. The light is concentrated at the core of the galaxy, with the brightness gradually diminishing towards the outer regions. There is a general lack of discernible spiral arm structure or prominent dust lanes. The galaxy displays a yellowish-white color gradient, likely indicating a population of older stars. A subtle distortion is visible on one side, suggesting a possible minor interaction with another celestial body. However, the overall morphology indicates a non-merging system. There may be some ongoing star formation based on a hint of bluer light in the outer regions, although the galaxy primarily appears to consist of an older stellar population.
