The galaxy presents as a single, relatively smooth object. Its morphology is predominantly elliptical or spheroidal. There is no clear spiral arm structure or evidence of a distinct disk. The light distribution is centrally concentrated, exhibiting a smooth gradient outwards from the core. The galaxy is roughly circular, with a slight deviation towards a prolate shape. There are no obvious signs of tidal tails, shells, or other features indicative of recent major mergers. The color profile suggests a population of relatively old stars, with a redder hue dominating the overall appearance. However, a small amount of bluer light may suggest some ongoing star formation, although this is not overtly apparent. There is no visual evidence of dust lanes or significant obscuration within the galaxy. Given its overall appearance, this galaxy is most likely an early-type galaxy with minimal recent interaction activity.
