The galaxy presents an overall smooth morphology, with a centrally concentrated bulge exhibiting a yellowish hue, likely indicating an older stellar population. The surrounding disk shows a bluish tint, suggesting the presence of younger, hotter stars and possibly ongoing star formation, albeit at a moderate rate. The galaxy's shape appears to be transitioning between round and elliptical, lacking any strong evidence of distinct spiral arms or a prominent bar structure. There are no visually apparent signs of major mergers or tidal disturbances. Minor asymmetry suggests a weak interaction or some internal disturbance.
