The galaxy exhibits a generally smooth morphology, with a slightly elongated, possibly elliptical shape. There is some evidence of internal structure, including a brighter, concentrated core region. Fainter, diffuse emission extends outward from the core, appearing somewhat patchy and uneven in distribution. The galaxy's color appears relatively red, indicating an older stellar population and/or significant dust content. There may be some minor tidal disturbances or interactions occurring, as hinted by subtle asymmetries in the outer regions. However, there is no definitive evidence of a major merger event based on this image alone. The overall appearance suggests an evolved system, possibly an elliptical galaxy, but further spectroscopic or photometric data would be needed for more precise classification.
