This galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The light distribution is centrally peaked and gradually diminishes outwards. Its shape appears to be moderately elliptical, leaning towards a spheroidal form, with no distinct spiral arm features visible. Color gradients suggest an older stellar population, with a yellowish-red hue dominating the inner regions. No obvious signs of active star formation are discernible from the image alone, consistent with a relatively quiescent state. There is a subtle asymmetry. The galaxy appears to be isolated with no significant tidal disturbances or signs of ongoing mergers detected in this image.
