The galaxy presents as a slightly elongated, disk-like structure with a notable central bulge. The light distribution appears relatively smooth, suggesting an absence of prominent spiral arms. The color profile indicates a possible population of older stars, contributing to the galaxy's overall hue. There appears to be some minor disturbance of the light suggesting tidal interactions with another galaxy. The galaxy's estimated size appears relatively compact. The object appears to be undergoing a relatively low rate of star formation.
