The galaxy appears to be a lenticular or early-type spiral, exhibiting a dominant, smooth bulge component. It shows a slightly elongated shape, displaying an intermediate degree of roundness. There is evidence of a faint, disklike structure surrounding the bulge, though it is not well-defined. The galaxy appears to be primarily smooth, with some minor features that could indicate minor disturbances or interactions. The central region exhibits a brighter concentration, possibly indicative of an active galactic nucleus or a dense stellar population. The color profile suggests a population of older stars dominating the bulge, with a relatively small amount of ongoing star formation in the disk, showing up as some pockets of redder color. Overall, the galaxy appears to be relatively massive with moderate star forming properties.
