The galaxy presents a generally smooth morphology, with a slight elongation suggesting a prolate spheroidal shape. The central region exhibits a concentrated, yellowish-orange hue, indicative of an older stellar population. Moving outward from the core, a faint, greenish halo is observed. The overall structure appears relatively undisturbed, with no strong evidence of tidal tails or major merger activity. Faint, diffuse features are present, possibly representing weak spiral arms or star-forming regions. The galaxy has a relatively low star formation rate.
