The galaxy presents a morphology that appears to be between smooth and disk-like. The central bulge region exhibits a concentrated, bright luminosity with a yellowish hue, suggesting a population of older stars. Extending from the central bulge is a fainter, diffuse region that may indicate the presence of a disk component. While a defined spiral structure is not readily apparent, there are hints of features or disturbances extending from the central region. The overall shape of the galaxy is neither perfectly round nor elongated, showing an intermediate form. There appears to be some minor disturbance, perhaps a sign of minor interaction. The galaxy displays a blue tint around the edges, which could signify ongoing or recent star formation activity. 
