This galaxy exhibits a morphology suggestive of a disk galaxy, though the image resolution limits detailed characterization of spiral arm structure. The central bulge appears prominent and possesses a yellowish hue, potentially indicating an older stellar population. A flattened disk structure is observed extending outward from the bulge. The disk displays a bluish tint, hinting at the presence of younger, hotter stars and ongoing star formation, though at a relatively low rate. There is also evidence of a slight warp or disturbance in the disk's symmetry. The galaxy appears to be somewhat inclined with respect to our line of sight, preventing a full face-on view. The overall shape of the galaxy is somewhere between round and cigar shaped. No clear signs of a major merger are observed, but minor disturbances can be noted.
