The galaxy presents as a relatively smooth, elongated structure, consistent with a disk galaxy viewed at an oblique angle. The central bulge is prominent and appears yellowish-orange, suggesting an older stellar population. There's a subtle color gradient as we move outward from the core, with the disk appearing slightly bluer or greener. This may indicate the presence of younger, hotter stars and ongoing star formation in the outer regions, though at a relatively low rate. The galaxy lacks any clear spiral arm structure and has no strong disturbances, indicating it is not currently undergoing a major merging event. The overall shape is more lenticular, indicating a relatively evolved system.
