The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The light profile appears centrally concentrated, fading gradually towards the outer regions. The color gradient suggests a population of older stars dominating the central bulge, appearing more yellow/red, possibly indicating lower levels of recent star formation. A slight blue tinge on the outer edges could indicate a younger stellar population. The galaxy appears to be relatively isolated, showing no signs of major interaction with other galaxies or significant tidal disturbances. It appears nearly round, with no significant elongation or disk-like structure visible. There might be the slightest indication of a minor disturbance, though further analysis would be required.
