This galaxy presents an elliptical morphology. It exhibits a smooth, centrally concentrated light distribution, with a high degree of central luminosity. The galaxy appears moderately elongated, with a noticeable tilt relative to our line of sight. A faint, diffuse halo surrounds the brighter central region. There is no evidence of distinct spiral arms or prominent dust lanes within the galaxy's structure, nor are there visible signs of tidal interactions or major mergers. The galaxy displays a redder hue, indicating a population of older stars.
