The galaxy presents a generally smooth and featureless appearance. Its shape is predominantly rounded, transitioning towards a more elliptical form along its major axis. There are no distinct spiral arms or bar structures visible. The central region exhibits a bright concentration of light, suggestive of a significant stellar population or potentially an active galactic nucleus. A subtle color gradient is observed, with a bluer hue present in the outer regions and a slightly redder tint concentrated towards the center. This may indicate younger stellar populations in the outskirts and older, redder stars dominating the core. No significant tidal features or distortions are apparent, implying it has not undergone any recent major mergers. However, some slight asymmetries in the outer regions could be indicative of minor gravitational interactions or past accretion events. Overall, the galaxy is likely an elliptical or lenticular type, exhibiting characteristics of a relatively evolved system.
