The galaxy presents as a largely featureless, elliptical morphology. A smooth, centrally concentrated bulge dominates the overall structure, with a noticeable radial decrease in surface brightness extending into the outer regions. There is little evidence of spiral arm structure or distinct dust lanes within the visible portion of the galaxy. The galaxy appears to be relatively round in shape. The color gradient suggests a population of older stars within the bulge, emitting a yellowish hue, while bluer colors towards the edges indicates the presence of a younger population there, though this is faint. There is no apparent evidence of active galactic nuclei activity or significant ongoing star formation, based on its appearance in the image. No tidal tails or distortions are visible, suggesting a relatively isolated system with no recent major merger events.
