The galaxy presents as a moderately compact object, exhibiting a generally elliptical morphology. It displays a concentrated central bulge, which appears to be a dominant feature, potentially indicative of an older stellar population. The light profile is generally smooth. There is a subtle hint of a surrounding disk-like structure, though this is not sharply defined and appears somewhat diffuse. Faint blue light is visible in the disk, which indicates ongoing, albeit low-level, star formation. There appears to be no significant sign of active galactic nuclei or strong tidal disturbances, though subtle asymmetries cannot be ruled out at this image resolution. Overall, the galaxy seems to be a relatively quiescent system with characteristics that align with an intermediate-mass galaxy undergoing subdued star formation.
