The galaxy presents an overall elliptical morphology, appearing largely smooth and relatively featureless in the observed light. The primary body exhibits a concentration of light towards the center, gradually decreasing in intensity outwards. The color profile suggests a dominant population of older stars, with a yellow to reddish hue indicative of lower star formation rates. There is evidence of a potential minor interaction or disturbance in the form of a smaller, separate, redder region offset from the galaxy's main body, possibly representing a dwarf galaxy in the process of merging or experiencing tidal disruption. The overall shape suggests a spheroid with only slight elongation.
