The galaxy presents a generally smooth morphology, with a subtle disk-like appearance. The light distribution suggests a concentration towards the center, indicative of a bulge component. The shape is more in-between than obviously round or cigar-shaped. There is no clear evidence of a major ongoing merger or significant tidal disturbance, although a subtle asymmetry might suggest a minor interaction in the past. The color indices suggest a redder population, potentially indicating a population of older stars and diminished star formation activity. The inferred mass indicates that this is a massive galaxy. 
