The galaxy presents as a relatively compact object, exhibiting a dominant smooth morphology. Its overall shape appears approximately elliptical, with an intermediate roundness. Faint tidal features may be present, but these are not definitive. The galaxy's color profile suggests a redder overall population, possibly indicative of an older stellar population and/or a significant dust component. Star formation appears to be suppressed. There is no clear evidence of a distinct disk structure within the resolution limits of the image. The galaxy may be in the process of, or recently experienced, a minor merger event.
