The galaxy presents a morphology consistent with an elliptical galaxy, displaying a relatively smooth and featureless light distribution. Its overall shape appears to be moderately elliptical, tending towards round. There is no obvious evidence of spiral arms, a central bar, or significant dust lanes. The galaxy exhibits a color gradient with a bluer core, indicative of a possible younger stellar population compared to the outer regions. There's no strong visual indication of an active galactic nucleus or a highly energetic starburst region. The light profile of the galaxy appears to fade gradually from the center outward, without any abrupt truncation. No clear signs of ongoing major mergers or strong tidal interactions with neighboring galaxies are evident.
