The galaxy presents as a spiral type, with a disk exhibiting a noticeable inclination relative to our line of sight. The spiral arms are tightly wound and somewhat difficult to resolve individually, suggesting a flocculent structure. The central bulge is moderately prominent and appears relatively smooth, contributing significantly to the galaxy's overall luminosity. There appears to be a weak bar structure present in the central region. The color distribution across the galaxy varies, with a bluer hue observed in the outer regions, possibly indicating ongoing star formation, while the central bulge exhibits a redder color, suggesting an older stellar population. The galaxy does not appear to be undergoing any major mergers or tidal disruptions, and the overall morphology seems relatively undisturbed.
