The galaxy presents as a well-defined elliptical structure. The light profile suggests a centrally concentrated bulge, with a smooth, gradual decrease in luminosity extending outwards. The core region exhibits a yellowish hue, possibly indicative of an older stellar population. The outer regions appear fainter and exhibit a slightly reddish tint. There are no prominent spiral arm features or dust lanes visible in this image. The overall morphology indicates a galaxy undergoing minimal star formation, with a significant proportion of the stellar mass residing in older populations. Subtle irregularities in the light distribution may suggest minor tidal interactions. The galaxy's shape is elongated, with a roughly 2 kpc radius.
