The galaxy exhibits a predominantly smooth morphology, with a high degree of central concentration. The light profile suggests a classification towards the elliptical or lenticular galaxy types. It presents with an intermediate ellipticity, appearing more oval than perfectly circular. The core displays a bright, concentrated yellowish hue, indicative of an older stellar population. Fainter, more diffuse extensions are observed along the major axis. These extensions exhibit a bluer tint, potentially indicating regions of more recent or ongoing star formation, or the presence of a more scattered population of stars. There is no apparent evidence of strong spiral arm structures, major mergers, or significant tidal disturbances. A minor asymmetrical feature is visible that might be indicative of a minor interaction or past tidal event. The galaxy is relatively compact, showing a moderate angular size in this image.
