The galaxy presents as a concentrated, elliptical-like structure. Its core appears very bright and somewhat unresolved, with a yellowish-orange hue, suggestive of an older stellar population. The galaxy appears largely featureless, lacking distinct spiral arms or a bar structure. There is a slight elongation to the galaxy's overall shape, though it appears mostly rounded. The outskirts of the galaxy gradually fade into the background, with no sharp edges or signs of tidal disturbances. There may be a very subtle ring-like structure partially visible around the central bulge, which appears bluer than the core. No distinct dust lanes or regions of intense star formation are readily apparent. There is no obvious evidence of a major ongoing merger, although subtle irregularities in the outer regions could indicate minor interactions in the galaxy's past.
