The galaxy presents as a generally smooth, elliptical-like structure with a concentrated central bulge. It exhibits a yellowish-orange color, suggesting a population of older stars. There appears to be a slight elongation, hinting at a possible deviation from a perfectly spherical shape, or potentially an edge-on disk. There is no clear evidence of spiral arms or significant dust lanes. A fainter, more diffuse halo may surround the central region. There are no strong indications of recent major merger activity, though subtle irregularities in the light distribution may indicate minor disturbances or past interactions.
