The galaxy presents as a single, largely featureless object with a concentrated central region. The color profile suggests an older stellar population, as indicated by the reddish-yellow hue, which fades towards the outer edges. There is no discernible spiral structure or distinct dust lane visible. The galaxy appears to be relatively smooth and elliptical in shape, although slight irregularities may exist at the periphery. The overall morphology is consistent with an early-type galaxy, possibly an elliptical or lenticular galaxy. The galaxy exhibits a gradual decrease in surface brightness from the core outwards. There are no obvious signs of ongoing major mergers or significant tidal disturbances.
