The galaxy presents as a largely featureless, smooth object with a concentrated central bulge. Its overall shape approximates circular symmetry, appearing nearly round. A slight elongation is potentially discernible, but it's subtle.

The color profile indicates a relatively red and old stellar population, especially within the core region, where a yellow-orange hue dominates. The outer regions show a slight bluer shift compared to the core, which suggests a possibility of younger stars residing within the outer regions.

There is no significant evidence of spiral arms, bars, or dust lanes characteristic of spiral galaxies. Nor are there indications of ongoing major mergers or substantial tidal disruptions. The galaxy appears largely undisturbed. Minimal potential structural asymmetry may exist.

