The galaxy presents an overall elliptical morphology, with a smooth, centralized bulge indicative of an older stellar population. The color profile suggests a mature galaxy, with a yellow-red hue dominant, likely due to the prevalence of red giant stars and lower levels of ongoing star formation. Some features, like a tidal tail, suggest there is a possibility of interaction with a second galaxy. The galaxy demonstrates no prominent spiral arm structure. There appears to be some dust obscuration within the main body. The overall luminosity implies a large mass.
