The galaxy presents a generally smooth and elliptical morphology. Its overall color is predominantly yellow, suggesting a stellar population dominated by older, redder stars. A slightly brighter, more diffuse region is present at the core, hinting at a possible active galactic nucleus or a higher concentration of stars. The galaxy does not exhibit any prominent spiral arms or distinct disk features. There is no strong evidence of ongoing major merging activity or tidal disturbances in its immediate vicinity, though some minor asymmetry cannot be completely ruled out. The galaxy appears relatively isolated, exhibiting a well-defined shape without significant elongation or irregular features. Its general roundness suggests it is being viewed from a position perpendicular to its rotation axis.
