The galaxy appears as a disk galaxy, inclined at a moderate angle to our line of sight. The central bulge is prominent, exhibiting a yellowish hue, suggestive of an older stellar population. Fainter blue arms or spiral structures are observed extending from the central bulge, these structures are very subtle however. The overall morphology can be described as elliptical. There is no clear evidence of a major ongoing merger event, though some minor disturbances in the morphology may indicate recent interactions or internal dynamical processes. It is difficult to definitively assess the presence of a bar structure from this image. The galaxy shows moderate luminosity with signs of faint star formation.