The galaxy presents as a relatively smooth and rounded object, exhibiting a primarily elliptical morphology. The light distribution appears concentrated towards the center, suggesting a prominent bulge. There is a slight color gradient visible, transitioning from a greenish hue in what appears to be the central region, toward a redder hue towards the outskirts of the galaxy. The galaxy does not display any apparent spiral arm structure or significant dust lanes. There is little to no evidence of tidal features or interactions with neighboring galaxies, suggesting it has not undergone a recent major merger. Small irregularities in the surface brightness are visible in the outskirts, perhaps resulting from minor interactions. The overall appearance indicates a galaxy dominated by an older stellar population, consistent with a low star formation rate.
