This galaxy presents a generally smooth, elliptical morphology. The light distribution is centrally concentrated, displaying a bright, well-defined core that diminishes outwards. The galaxy appears to be quite round in shape, lacking any significant distortion or tidal features suggestive of ongoing major interactions. There may be some minor features visible, though the general appearance would lead you to believe this galaxy is quite old.

Based on the color profile, the stellar population is likely a mix of older, redder stars contributing to the central bulge, with hints of younger, bluer stars in the outer regions, possibly indicating some ongoing, but modest, star formation activity. There is no obvious spiral structure or distinct dust lanes visible.
