The galaxy presents as an elliptical morphology. The central region appears as a concentrated spheroid of intense light, indicative of a dense stellar population, likely older stars. Proceeding outward, the light intensity decreases gradually towards the edges of the object. The overall color is yellowish-red, suggesting a low rate of star formation and a population dominated by older, redder stars. The isophotes exhibit a relatively smooth gradient, which suggests the galaxy is nearing completion of a merger or may be at a stage of equilibrium, without significant tidal features or disruptions. The disk ratio appears flattened, indicating a significant inclination with respect to the observer. The light distribution suggests a high Sersic index, which is common for elliptical galaxies. There is a possible slight warp to the galaxy's disk, but it may be an artifact.
