The galaxy presents a generally smooth morphology, appearing elliptical in shape. It displays a bright, concentrated central bulge, which transitions into a more diffuse, extended disk. The color gradient suggests a redder hue towards the core, potentially indicating an older stellar population. Fainter, bluer regions are observed in the outer disk, hinting at areas of ongoing or recent star formation, although at a relatively low rate. There is little to no visual evidence of spiral arm structure or major disturbances in the galaxy's overall form. It seems to be relatively isolated.
