The galaxy presents a generally smooth, elliptical morphology. The light distribution shows a concentration towards the center, forming a bright, yellowish core region. This core gradually transitions into a more diffuse, bluish halo extending outwards. There is a slight elongation in the galaxy's shape, deviating from a perfectly circular appearance. No distinct spiral arm structures are discernible, nor is there evidence of strong tidal features or ongoing major mergers. There may be some minor disturbance in the outer halo, possibly indicating a previous or ongoing minor interaction with a smaller galaxy. The colors suggest a stellar population composed primarily of older stars in the central region, with younger, bluer stars in the outer regions. The galaxy displays a moderate level of intrinsic luminosity.
