This galaxy appears to be a spiral galaxy, although the orientation makes it difficult to confirm the presence of well-defined spiral arms. It is seen at an oblique angle, potentially close to edge-on, and exhibits a bright central bulge with a slightly elongated disk. The bulge is characterized by a concentrated luminosity, indicative of a dense stellar population. The disk appears relatively smooth, with some faint diffuse light extending from the central region. There are some minor asymmetries, suggesting possible gravitational interactions or internal disturbances. The overall color suggests the presence of both older stellar populations in the bulge and some ongoing star formation within the disk.
