The galaxy presents as a relatively well-defined disk galaxy, viewed at an oblique angle. There is a notable central bulge exhibiting a concentrated luminosity profile, suggestive of a high stellar density. The disk component appears less defined, with a smoother texture and a yellowish hue overall, potentially indicating an older stellar population. Faint extensions are visible on either side of the central bulge, indicating what may be spiral arm structures. These arms appear tightly wound and relatively smooth. Additionally, there is a noticeable asymmetry in the disk's structure. It appears that the galaxy may be undergoing minor interactions or gravitational disturbances, based on slight warping of the disk plane. Star formation appears suppressed.
