The galaxy presents as a relatively smooth, elliptical structure, exhibiting a concentrated central bulge. The light profile suggests a high degree of sphericity with minimal indication of spiral arm structures or prominent dust lanes. A yellow-orange hue dominates the core region, likely indicative of an older stellar population. Fainter, more diffuse light extends outwards from the core, gradually fading into the background. The galaxy appears to be undergoing, or has recently undergone, a significant merger event. This galaxy presents an interesting example to study, as this appears to be a low star forming galaxy, which is quite interesting given its disturbed morphology.