The galaxy presents as a slightly elongated, disk-like structure viewed at a moderate inclination. The central bulge is prominent and exhibits a yellowish hue, suggestive of an older stellar population. The surrounding disk appears smoother and contains a mix of colors, with hints of bluer regions, possibly indicating areas of recent star formation. Overall, the galaxy appears relatively undisturbed with no obvious signs of a major merger event. It is characterized by a moderate size and luminosity, and the rate of star formation seems to be relatively low.
