The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth, symmetrical morphology. It presents as a diffuse, centrally concentrated object, with a luminosity profile that gradually decreases outwards from the nucleus. There is no apparent disk structure or spiral arm features visible. The core region exhibits a yellowish color, suggesting an older stellar population. The outer regions appear somewhat redder, potentially indicative of a continuation of aging stars and a lack of significant ongoing star formation. The galaxy's overall shape appears slightly elongated, falling somewhere in between a perfectly round and cigar shape. There is no obvious evidence of tidal tails, bridges, or other signs of recent major merger activity, although very slight asymmetry or disturbance could be present.
