The galaxy presents a largely smooth, rounded morphology with a concentrated central bulge. Its color profile indicates a mix of stellar populations, with a yellower hue dominating the core, suggestive of older, redder stars. Moving outward from the core, there appears to be a subtle transition toward bluer tones, which could indicate the presence of younger, hotter stars in the outer regions. No distinct spiral arm structure or bar features are discernible, implying a classification leaning towards elliptical or lenticular. There are no apparent signs of major disturbances or interactions with other galaxies. Faint features extend from the core, but are difficult to resolve with high confidence.
