The galaxy presents as a single, relatively smooth and concentrated light source, appearing largely elliptical or spheroidal in shape. Its core is bright and condensed, suggesting a high stellar density in the central regions. The intensity of the light appears to fall off gradually moving outward from the central bulge, indicating a relatively smooth distribution of stellar populations within the galaxy. There are hints of a faint extended halo around the galaxy, though the boundaries are not well-defined. Overall, it appears to be a largely undisturbed system, without any major signs of ongoing mergers or tidal interactions. There are no prominent spiral arms or other distinct features typically associated with disk galaxies.
