The galaxy presents as a centrally concentrated object with a generally smooth morphology. There's a slight elongation, not quite cigar-shaped, leaning more toward an elliptical form than a flattened disk. Faint, diffuse outer regions are visible, suggesting a gradual decline in stellar density from the core. No prominent spiral arms or bar structures are discernible. The galaxy exhibits a yellowish hue, with some suggestion of bluer regions present in low fractions. No signs of major mergers or significant tidal disturbances are immediately apparent, although some minor disturbances cannot be ruled out given the resolution.
