The galaxy presents a generally smooth appearance, suggesting an elliptical or lenticular morphology. The central region exhibits a high concentration of light, appearing as a bright, nearly spherical core. Moving outward, the luminosity gradually decreases, but the gradient does not appear perfectly smooth. There is faint evidence of possible disrupted structures or tidal features.

Color gradients are present. The central bulge exhibits a yellowish hue, potentially indicative of an older stellar population. Fainter, bluer regions are subtly visible in the surrounding areas, hinting at the presence of younger stars or ongoing star formation at the edges. 

The overall shape is somewhat elliptical. Although the majority of the light is concentrated in the spherical core, some slight elongation and faint features could indicate an ongoing interaction or recent merger event.
