The galaxy presents as a lenticular or early-type spiral galaxy seen at an oblique angle. The central bulge is prominent and displays a bright, nearly uniform luminosity profile, suggesting an older stellar population and a lack of significant dust obscuration. The disk component is visible but appears relatively smooth with limited discernible spiral arm structure. There is a slight elongation visible, hinting at a possible bar structure or tidal interaction, though no strong visual distortions are evident. The galaxy exhibits a blueish hue, possibly indicative of ongoing star formation. Overall, this galaxy seems to be in a relatively evolved state, with star formation occurring at a fairly low rate. No clear signs of major merging activity are observable.
