The galaxy presents as a relatively smooth, disk-like structure seen at a moderate inclination. The central bulge is prominent, exhibiting a bright, concentrated luminosity profile. The color appears to be generally redder, especially in the central region, suggesting an older stellar population. The disk shows only faint, subtle features, indicating a lack of significant spiral arm structure or prominent star-forming regions. There is a small, disturbed area to the upper left of the galaxy indicating the possibility of minor merging with another object. Overall, the galaxy appears to be a relatively evolved system, possibly an early-type spiral galaxy.
