The galaxy presents as a relatively compact, disk-shaped structure. The central bulge appears prominent and exhibits a yellowish hue, suggesting a population of older stars. A flattened disk surrounds the bulge. The disk shows hints of spiral arm structure, but these are not well-defined or tightly wound. There is a faint blue tint in the outer regions of the disk, potentially indicating regions of more recent star formation. The overall structure is somewhat elongated and classified as cigar shaped, as it is not perfectly circular, but generally smooth. There does not appear to be any evidence of a major ongoing merger or strong tidal disturbances in this image, but there appears to be minor disturbances.
