The galaxy presents a somewhat elliptical morphology, lacking defined spiral arms. Its light is concentrated towards the center with a prominent bulge exhibiting a yellow hue, suggesting an older stellar population. The outer regions of the galaxy show a bluer tint, indicative of ongoing or recent star formation, though this region is fairly faint. There is a minor amount of apparent disturbance in the morphology, but no obvious signs of a major merger event. Overall, the galaxy seems to exhibit characteristics of both elliptical and spiral galaxies, perhaps representing an intermediate stage or a galaxy that has undergone past interactions. The galaxy is moderately luminous, with a substantial mass. It has a relatively low star formation rate and specific star formation rate.
