The galaxy presents an overall elliptical morphology, elongated with an aspect ratio suggesting a moderate degree of flattening. The light distribution appears relatively smooth, lacking distinct spiral arm structures or prominent dust lanes. The central region exhibits a higher surface brightness, indicative of a concentrated nucleus or bulge. Color gradients across the galaxy are subtle, with a slightly redder hue towards the central bulge and a marginally bluer tint in the outer regions, potentially indicating a radial variation in stellar populations or star formation activity. There appears to be only a very slight disturbance in the main structure of the galaxy. The estimated half-light radius is a few kiloparsecs, suggesting a galaxy of moderate physical size.
