The galaxy exhibits a somewhat elliptical morphology. The central region presents a yellowish-orange hue, potentially indicating an older stellar population or significant dust obscuration. Surrounding the core, the galaxy displays a bluer component, which may suggest regions of more active star formation. There are noticeable irregularities in the distribution of light, with some areas appearing more diffuse and extended. While not perfectly spherical, the galaxy lacks a clearly defined disk structure, and there are indications of tidal features or interactions, possibly indicative of an ongoing or recent merger event. The galaxy shows signs of star formation, although the yellow/orange hue in its center means it probably is older.
