The galaxy appears to be a spiral galaxy viewed at an oblique angle. The central bulge exhibits a concentrated luminosity, suggesting a significant population of older stars. Evidence of a disk is visible, presenting a mottled texture indicative of ongoing star formation. The spiral arms are not well-defined, appearing somewhat flocculent. The galaxy's shape is primarily elliptical. There's a suggestion of minor disturbances in the disk structure, possibly due to a past interaction or merger. The overall color profile of the galaxy is mixed, with the central bulge exhibiting a yellower hue and the disk regions exhibiting a bluer hue. The lack of obvious dust lanes suggests the galaxy is observed at a relatively late stage of its evolution. Overall, the galaxy appears to be intermediate in mass.
