The galaxy presents as a largely featureless, elliptical morphology. The light distribution is centrally concentrated, showing a smooth gradient outward from a bright core. The primary color of the galaxy is a warm, yellow-orange hue, indicative of an older stellar population. There is a subtle color gradient within the galaxy, with the central regions appearing slightly more yellow, and the outer regions trending towards a more red hue. This suggests that the star formation has largely ceased, with older, redder stars dominating the light output, particularly in the outskirts. The galaxy appears relatively isolated and undisturbed, with no clear signs of recent major mergers or tidal interactions. There may be faint hints of a very weak, diffuse halo extending outwards, but this is difficult to discern definitively. There are no apparent dust lanes or spiral arm structures visible.
