The galaxy presents a somewhat elongated morphology, appearing disk-like, with a central bulge that dominates the light profile. The bulge exhibits a bright, concentrated core region. Surrounding the central bulge, a fainter and more diffuse disk structure is observed. The galaxy appears slightly disturbed, possibly indicating a minor interaction or merger event. The optical color profile suggests a significant population of older stars, along with regions that display characteristics associated with younger, bluer stellar populations. The overall structure is generally consistent with a late-type spiral, potentially an irregular galaxy.
