This galaxy appears to be a relatively smooth system, exhibiting a central bulge with a noticeable disk. The bulge displays a yellowish-white hue, suggesting an older stellar population. The disk surrounding the bulge shows bluer regions, potentially indicating areas of more recent star formation. The disk appears moderately inclined relative to our line of sight, revealing a somewhat flattened shape. There is a subtle asymmetry in the outer regions of the galaxy, hinting at a possible minor interaction or disturbance. The galaxy shows limited signs of spiral arm structure, although faint, diffuse features are visible in the disk. The system does not exhibit any prominent tidal tails or strong indications of a major merger event, though a slight distortion is present. The overall color suggests intermediate levels of star formation activity.
