The galaxy exhibits a primarily smooth morphology, with a centrally concentrated light profile. The overall shape is somewhat elongated, approximating an elliptical form, although it does not appear perfectly spherical. There is little evidence of distinct spiral arms or prominent disk structures; the galaxy appears more spheroid in nature. Color gradients are present, with a yellowish-orange hue dominating the core region, suggesting an older stellar population. The outer regions show a bluer tint, albeit subtle, potentially indicating the presence of younger stars, or perhaps dust. There are no obvious signs of major mergers or significant tidal disturbances within the galaxy's visible structure, although minor asymmetry is present. Overall, the galaxy presents characteristics consistent with a relatively massive, evolved system.
