The galaxy presents as a relatively smooth, elliptical or lenticular system. Its overall shape is slightly elongated rather than perfectly spherical, appearing more akin to an oblate spheroid. The light distribution suggests a centrally concentrated bulge, brightest in the galaxy's core and fading gradually outwards. There is little evidence of spiral arm structures or significant dust lanes. Faint tidal features or minor disturbances might be present, though these are difficult to definitively confirm.

The galaxy's color profile appears largely homogenous, with subtle variations in hue across the body. The dominant color is a yellowish white, suggestive of an older stellar population dominated by lower-mass stars. Star formation may still be occurring, though it does not appear to be a dominant process. Overall, the galaxy presents as a relatively evolved system with a moderate stellar mass.
