This galaxy exhibits a generally smooth morphology, suggesting a classification as an elliptical galaxy or a lenticular galaxy viewed face-on. The light is concentrated towards the center, forming a bright, prominent bulge. The color profile indicates a significant population of older stars, as evidenced by the yellow-red hue, which could indicate that star formation is not currently a dominant process within the galaxy, though there is a hint of bluer hues on the outer edges. There is no obvious dust lane or spiral arm structure visible in the image. There appear to be some minor distortions in the outer halo, perhaps indicative of a past merger event or gravitational interaction.
