The galaxy presents as a relatively smooth, elliptical-like structure with a soft, diffuse appearance. There is a noticeable central bulge. The color profile suggests a moderate population of older stars, with a subtle gradient towards bluer hues in the outer regions. This hints at some ongoing, albeit low, star formation activity. There are subtle hints of disturbances within the galaxys morphology suggesting a possible minor interaction. The overall shape is neither perfectly spherical nor elongated into a disk, but rather an in-between form. The galaxy is estimated to be of moderate mass.
