The galaxy exhibits a somewhat elongated morphology, potentially indicating an elliptical shape. A significant portion of its light is concentrated in the central region, suggesting a prominent galactic bulge. The galaxy displays a relatively smooth texture, lacking distinct spiral arm structures. Color gradients are observed, with a shift toward redder hues in the central regions, possibly indicative of an older stellar population, compared to bluer, younger stars in the outer regions. There may be a second galaxy in the process of merging with it, or two seperate galaxies in close proximity. There is some mild tidal distortion.
