This galaxy presents as a relatively smooth, centrally concentrated object. The overall color suggests a population of older stars, with a generally redder hue compared to galaxies with more active star formation. There is a slight elongation, though the galaxy appears mostly round. No distinct spiral arms or bar structures are discernible. There is some evidence of faint, extended diffuse light surrounding the main body of the galaxy. Based on these observations, this is likely an elliptical or lenticular galaxy. The absence of strong blue color or features associated with gas or dust suggests a low rate of star formation. There are no obvious signs of recent or ongoing major mergers or tidal disturbances that might disrupt its smooth morphology, although a minor interaction cannot be ruled out due to some slight asymmetry and faint disturbances in its light profile.
