The galaxy presents as a concentrated, centrally brightened object with a smooth overall morphology. The core exhibits a yellowish-white hue, indicative of an older stellar population. Moving outward from the core, the color transitions toward a slightly greener tint, potentially suggesting the presence of some younger stars or regions of ongoing, albeit limited, star formation within the galaxy's outer regions. The galaxy appears relatively undisturbed, without any significant signs of tidal interactions or mergers. It exhibits a somewhat elliptical shape, leaning toward being moderately rounded, rather than a highly elongated or cigar-shaped appearance. There is no clear spiral arm structure or a well-defined disk visible. The outskirts of the galaxy gradually fade into the background, lacking any distinct, sharp boundaries.
