The galaxy presents a generally smooth, elliptical morphology. Its central region exhibits a concentrated, bright core radiating primarily in the redder wavelengths, suggesting a significant population of older stars. The overall color profile indicates a relatively quiescent galaxy with limited ongoing star formation. The isophotes appear relatively round, with only subtle deviations from perfect circularity. There is no obvious evidence of spiral arm structure or significant dust lanes. No major merger events are apparent, although there is a slight suggestion of minor gravitational disturbance in the outer regions, but not definitive. The galaxy extends a significant distance, spanning over 11 kiloparsecs.
