The galaxy appears to be relatively compact, presenting a morphology suggestive of an early-type system. The light distribution is somewhat smooth, with a general spheroidal shape but with irregular features. The galaxy core shows a bright central region, with the overall color profile exhibiting a variation in spectral characteristics. Some areas are dominated by redder hues, indicative of an older stellar population, while the core shows bluer tones. These bluer tones indicate the presence of younger, hotter stars. There is some indication of disturbances in the outer regions that point toward a possible interaction with another galaxy or a previous merger event. These disturbances distort the overall symmetry of the galaxy. The overall shape of the galaxy does not lend itself towards a classification as a spiral galaxy, and there is no prominent spiral arm structure.
