The galaxy presents an overall elliptical morphology, with a dominant, centrally concentrated bulge. The core exhibits a bright, yellowish hue, suggesting an older stellar population. Fainter, diffuse extensions are visible along the equatorial plane, hinting at a possible disk component or tidal features. There is some irregularity in the outer regions. It appears to be undergoing some sort of interaction. The overall color is red, possibly indicating a high degree of dust obscuration or a population of older stars. There are also blue regions, which are possible areas of star formation.
