The galaxy presents a largely smooth, elliptical morphology. The galaxy core exhibits a bright, concentrated luminosity profile, indicative of a substantial central mass concentration. The galaxy appears relatively compact, with a diameter of approximately 6 kiloparsecs. The light distribution suggests an evolved stellar population, with a dominant redder hue, although the inner core appears to be relatively blue, indicative of some active star formation, but at a relatively low rate. There is little evidence of significant ongoing major merging events, but a minor disturbance may be present in the galaxy's morphology. The galaxy is mostly rounded in shape, with little deviation from ellipticity.
