The galaxy presents as a lenticular, disk-shaped structure with a smooth, centrally concentrated bulge. It has a moderate inclination relative to our line of sight, which allows some visualization of its disk. The bulge appears to be largely featureless, indicative of an older stellar population. The disk component shows a faint, diffuse structure, with limited evidence of defined spiral arms or prominent star-forming regions. The overall color profile suggests a predominantly evolved stellar population. There is no apparent major disruption of the galaxy's structure, suggesting it is relatively isolated.
