The galaxy appears to be a relatively smooth, elliptical-like object with a concentrated central bulge. The light profile suggests a gradual decrease in brightness from the core outwards, with no prominent spiral arm features visible. A slight elongation is observed, deviating from a perfectly circular shape. The color is somewhat uniform, with a yellow-white hue, characteristic of an older stellar population. No significant dust lanes or star-forming regions are apparent upon visual inspection. The overall morphology indicates a mature galaxy, potentially an elliptical or S0 type, without signs of recent major mergers, although subtle disturbances cannot be entirely ruled out.
