The galaxy presents as a slightly elongated, lenticular-like structure. It exhibits a bright, concentrated central bulge region, suggesting a significant population of older stars. A faint, disk-like component surrounds the bulge and is oriented roughly horizontally across the image. The disk appears relatively smooth, with minimal evidence of distinct spiral arm features, and a slight green tinge in the color. The overall color profile indicates the presence of both older stellar populations in the central bulge and perhaps some ongoing, though subdued, star formation activity within the disk. The galaxy doesn't appear to be undergoing any major mergers or significant tidal disturbances, although there is a subtle asymmetry in the light distribution, possibly indicating a minor interaction.
