The galaxy presents a largely smooth, elliptical morphology. Its central region exhibits a high degree of concentration with a bright core that transitions smoothly into an extended halo. The light distribution is fairly symmetrical. There is little indication of spiral arm structures or prominent dust lanes. The color profile appears relatively uniform across the galaxy, suggesting a stellar population dominated by older, evolved stars. The overall color indices are consistent with a redder, more passive galaxy compared to actively star-forming systems. There is no obvious evidence of ongoing major mergers or tidal disturbances, though a slight asymmetry is visible upon closer inspection. The galaxy's morphology suggests it is a relatively undisturbed system that has likely undergone significant evolutionary processing.
