The galaxy presents a generally smooth appearance with a slightly elliptical morphology. The light distribution is concentrated towards the center, suggesting a substantial bulge component. There is faint color variation across the galaxy, shifting from slightly yellower hues in the core to subtly redder tones in the outer regions. This color gradient might be indicative of older stellar populations dominating in the central regions, or dust obscuration effects. There is a slight asymmetry noticeable, giving a sense that it may have undergone a minor interaction sometime in the past.
