The galaxy presents as a multi-component system. The primary component appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated light profile. The color is generally yellowish, suggestive of an older stellar population with lower star formation activity. A secondary component is observed to the immediate northeast. This component has a bluer color, indicating ongoing star formation and a younger stellar population. This blue light is less concentrated. Based on the proximity and the disturbed morphology of the surrounding diffuse light, the system appears to be undergoing an active merger or tidal interaction. There are no obvious spiral arm structures visible in the primary body. The overall shape exhibits a moderate degree of ellipticity rather than a perfectly circular appearance.