The object presents as a galaxy with a generally smooth morphology, although some irregularities are visible. The galaxy exhibits a mostly elliptical shape. Its light profile appears concentrated, with a bright central region. The color gradient suggests a population of older stars dominating the light emission. There is little to no indication of active star formation regions. The galaxy exhibits signs of a possible merger or interaction, with a double nuclei being present in the center of the galaxy. This is characterized by 2 distinct bright cores within the central region of the galaxy. There is little evidence of a disk component or spiral arms. The overall size appears to be relatively large, suggesting a massive galaxy.