The galaxy exhibits a generally smooth morphology, suggesting it is likely an elliptical or lenticular type. A significant fraction of the galaxy's light is concentrated in a central bulge, which appears largely spheroidal. There are no prominent spiral arms or significant dust lanes visible in the image. The color profile indicates a population of older stars, particularly within the bulge, inferred from the reddish-yellow hue. The outer regions of the galaxy present a fainter, more diffuse glow. There is little evidence of ongoing major star formation within this galaxy. The galaxy appears isolated, with no obvious signs of a recent or ongoing merger event or major tidal disturbances. The shape of the galaxy appears generally round, with very little angularity.
