The galaxy presents a primarily smooth morphology, appearing elliptical in shape. The light distribution indicates a high degree of central concentration, with the luminosity decreasing gradually from the core outwards. There is a slight elongation, but the galaxy appears mostly rounded. The color profile shows a general redder hue, with the central regions appearing more yellow. No distinct spiral arms or bar structures are discernible. There is no clear evidence of any active merging or tidal disturbances. Overall, the galaxy appears to be a relatively evolved system, possibly with a population dominated by older stars and a low rate of on-going star formation.
