The galaxy presents as a primarily smooth, elliptical structure. The light distribution shows a concentrated central bulge that gradually diffuses outward, transitioning into a fainter halo. The overall shape is elongated, appearing as an ellipse with an intermediate ellipticity. There's little to no evidence of spiral arms or significant dust lanes. The color profile suggests a population of older stars dominating the galaxy's composition. The overall morphology indicates a galaxy that is not undergoing a major merger, though subtle disturbances could be present.
