The galaxy presents as a somewhat elliptical, disk-like structure with a moderately smooth appearance. Its central region displays a brighter, concentrated luminosity, suggesting the presence of a galactic bulge. The overall color profile appears to be a slightly bluer hue, especially towards the central area, with the color becoming redder in the outer regions. The edges of the galaxy are not sharply defined, indicating a gradual decrease in stellar density. There are some faint, irregular features apparent, potentially suggestive of minor disturbances or ongoing interactions, though a significant merging event is not obvious. Star formation may be present, but appears to be relatively low.
