The galaxy presents an elliptical morphology, exhibiting a generally smooth light distribution with a high degree of central concentration. There may be a slight deviation from perfect ellipticity, possibly indicating a subtle disk component or minor interaction. The color profile suggests a population of older stars, as inferred from the relatively red hue, particularly in the central regions. The surrounding halo appears fainter and somewhat bluer, indicative of a possible younger stellar population or recent minor merger activity in the outer regions. Overall, the galaxy seems to be a relatively massive system undergoing moderate star formation.
