This galaxy presents as an elliptical morphology with a relatively smooth appearance, showing minimal distinct features such as spiral arms or prominent dust lanes. It exhibits a central bulge that appears yellowish, indicative of an older stellar population. The outer regions of the galaxy display a bluer hue, suggesting the presence of younger, hotter stars, though this is less pronounced compared to galaxies with active star formation. The overall shape is somewhat elongated, deviating from a perfectly circular form. There's no evidence of ongoing major mergers or significant tidal disturbances, though a slight asymmetry may point towards minor interactions in its past or present. The outer edges of the galaxy fade gradually, indicating a smooth transition in stellar density.
