The galaxy presents as a relatively smooth, singular object with a general elliptical morphology. The central region exhibits a bright, concentrated luminosity. The galaxy displays a slight elongation, deviating marginally from a perfectly circular shape.  There is some indication of a minor disturbance in the galaxy's structure, potentially due to an ongoing or past interaction. The overall color suggests a population of older stars. The galaxy appears to be well-defined with a gradual decline in luminosity from the core outwards. 
