The galaxy presents as a centrally concentrated object, exhibiting a largely smooth morphology. The central region displays a high degree of luminosity, suggesting a significant stellar population density. The shape is generally elliptical but not perfectly so, with some deviation towards an intermediate state. There is a slight indication of minor tidal disturbances in the outer regions, though the overall structure appears relatively undisturbed. The galaxy exhibits a color gradient, transitioning from a more yellowish hue in the core to slightly redder tones towards the periphery. This color variation may indicate differences in stellar population ages and compositions, with older, redder stars dominating the outer regions. There is another faint, diffuse object in the lower left of the image that may be a dwarf galaxy.
