The galaxy presents as a relatively smooth, centralized light distribution with a slight elongation, deviating marginally from a perfectly circular form. It displays a prominent central bulge that contributes significantly to the overall luminosity. The outer regions fade gradually into the background, exhibiting a diffuse halo. A subtle hint of spiral structure or a disk component is suggested by a slight flattening. The galaxy's color profile shows a bluer hue in the central region, possibly indicative of recent star formation. There is an indication of a minor disturbance or interaction, with some asymmetry observed in the distribution of light.
