This galaxy appears to be an elliptical galaxy, exhibiting a smooth, diffuse light distribution. The morphology is generally featureless with no apparent spiral arms or distinct structures. The galaxy is elongated in shape, suggesting an E4 or E5 classification on the Hubble sequence. The core region is characterized by a high surface brightness, which gradually decreases towards the outer edges. There are hints of some tidal disturbances that may be influencing the overall structure. The galaxy's light appears more intense towards the center, indicating a concentration of stars in the nucleus. Color gradients within the galaxy are subtle, with a slightly bluer hue towards the outer regions. The overall color index suggests an older stellar population. The object presents no clear indications of ongoing major merger activity, although some minor interactions might be present.