The galaxy presents as a somewhat elliptical, disk-like structure, viewed at an angle that is not quite face-on. The central bulge appears relatively prominent and exhibits a smooth, concentrated distribution of light, suggesting an older stellar population. Moving outward from the bulge, the disk shows a gradual decrease in surface brightness. The overall color profile indicates a tendency towards redder hues, which may be related to an older stellar population. The galaxy has a moderately low star formation rate, evidenced by the absence of bright, blue star-forming regions. The outer regions of the disk show hints of asymmetry or minor disturbances, with the galaxy seemingly non-isolated, possibly hinting at past interactions.
