The galaxy appears to be an elliptical galaxy, exhibiting a smooth, featureless morphology with a concentrated central bulge. The light distribution is centrally peaked, suggesting an older stellar population with minimal ongoing star formation. It has a generally elliptical shape, with the ratio of the major to minor axis close to one. There are no clear signs of spiral arms, a bar, or any significant dust lanes. The core of the galaxy shows a yellowish/red hue, indicative of older stars, while the outer regions show a slight bluer tint. The galaxy appears to be an isolated object and does not show any major signs of tidal disturbances, such as tidal tails or bridges, implying that it is not currently undergoing a major merger. However, there may be minor perturbations indicating a minor disturbance, possibly caused by a past merger or accretion event.
