The galaxy presents as a relatively smooth, rounded structure with a concentrated central bulge. The color profile suggests a population of older stars, with a general yellow-red hue dominating the galaxy's light output. There is little evidence of ongoing, significant star formation based on the absence of strong blue or ultraviolet signatures in the image. The lack of spiral arm structures or prominent dust lanes further supports a classification towards the elliptical or lenticular type. The galaxy appears to be relatively undisturbed, showing no obvious signs of tidal interactions or major mergers, maintaining a largely homogenous and symmetrical appearance.
