The galaxy presents as a smooth, elliptical structure. Its shape is elongated, appearing somewhat cigar-shaped. The central region exhibits a higher surface brightness, indicating a concentration of stars and likely a supermassive black hole. The galaxy’s color appears generally yellowish-white, suggesting a population of older stars and reduced ongoing star formation. There is no apparent spiral arm structure or prominent dust lanes. The overall morphology suggests a relatively evolved system with a quiescent star formation rate. There is no clear visual evidence of any recent major merger activity or significant tidal disturbances within the immediate vicinity. The galaxy appears to be relatively isolated and undisturbed.
