The galaxy presents an elliptical morphology, elongated along its major axis with an apparent axis ratio of approximately 0.67. A distinct central bulge is visible, appearing smooth and concentrated, exhibiting a yellowish hue indicative of an older stellar population. The surrounding disk, which is less prominent, shows a bluer color, suggesting the presence of younger stars and ongoing star formation, although at a relatively low rate. Some minor disturbances appear in the outer disk, but are not suggestive of any recent major mergers. The galaxy appears relatively undisturbed and isolated. It is moderately luminous, with an estimated size that appears to be around 5.6 kpc.
