The galaxy appears to be an elliptical galaxy, characterized by a smooth, diffuse light distribution with no obvious spiral arms or disk-like structures. It exhibits a centrally concentrated brightness profile, diminishing gradually outwards. The core region displays a yellowish hue, suggestive of an older stellar population with a lower rate of star formation. The galaxy appears to be generally undisturbed, showing little evidence of recent mergers or tidal interactions. Its overall morphology is well-rounded, lacking any significant elongation or asymmetry.
