The galaxy appears as a singular, diffuse object. It presents an elliptical morphology, exhibiting a smooth, largely featureless profile, with no spiral arm structures readily discernible. There is no obvious central bulge or bar. The overall shape suggests a system that is closer to being in between round and cigar-shaped. The light distribution is centrally concentrated, and there is no evidence of strong tidal features or ongoing major mergers. Subtle colour variations can be observed within the galaxy's body, ranging from redder to bluer hues, possibly indicating variations in stellar populations or dust content, but the image quality limits a more detailed analysis of the features. There may be evidence of some minor disturbance, though this is not obviously distinguishable from the galaxy's main structure. 
