The galaxy presents as an elongated structure, appearing largely smooth with a concentrated central bulge. The light distribution suggests a dominant spheroidal component. There is faint evidence of a disc component extending outwards. The color profile indicates a redder core, potentially indicative of an older stellar population and dust obscuration. While the galaxy exhibits an overall smooth appearance, subtle asymmetries in the outer regions hint at possible interactions or minor disturbances, though no prominent tidal features are discernible within the limitations of this image resolution.
