The galaxy presents as a relatively smooth, elliptical-like structure, exhibiting a central bulge with a noticeable concentration of light. The overall color appears to shift from a warmer, reddish hue in the central region to cooler, bluish tones toward the outer edges. This color gradient may indicate a change in stellar populations, with older, redder stars dominating the core and younger, bluer stars populating the outskirts. The galaxy displays a moderate elongation, suggesting it is not perfectly spherical. There appears to be some minor asymmetry or faint disturbances in the outer regions, potentially hinting at past interactions or mergers, but these are subtle. The overall morphology suggests a galaxy that is undergoing relatively passive evolution, but the slight disturbances could suggest otherwise. Further investigation with higher-resolution imaging and spectroscopic data would be necessary to confirm the presence and nature of these subtle features.
