The galaxy presents a generally elongated, cigar-shaped morphology. It appears relatively smooth in overall structure, with a noticeable central bulge. The color distribution suggests a redder core region, potentially indicating an older stellar population. There also appears to be some slight asymmetry or a minor disturbance, but for the most part the galaxy appears relatively undisturbed, and has some potential disk features. This galaxy is likely to be a late type spiral galaxy. The apparent size, combined with its inferred distance, indicates that this is a moderate-sized galaxy. Based on its estimated size, it is consistent with a typical disk galaxy. Overall, this galaxy presents as a relatively quiescent system, with possible low rates of star formation.
