The galaxy presents as a relatively compact object with a slightly elongated morphology. The light distribution appears dominated by a smooth, centrally concentrated bulge component with a hint of an extended disk. The color gradient suggests a yellowish-orange hue, possibly indicating an older stellar population. There appears to be some asymmetry or disturbance in the light distribution, potentially indicative of tidal interactions or ongoing merger activity. There are subtle hints of faint, diffuse features extending from the main body of the galaxy.
