The galaxy appears as a single, relatively bright object with a smooth and somewhat diffuse profile. It exhibits an elliptical morphology, appearing more elongated than perfectly circular, though it lacks a pronounced cigar-like shape. There is an apparent tidal interaction or merger in progress. Two distinct but overlapping nuclei or brightness concentrations are visible within the main body, hinting at a merging event. The overall color appears yellowish-red, suggesting an older stellar population and lower levels of ongoing star formation. There are no prominent spiral arm structures or distinct features indicative of active star formation regions visible within the available resolution. The galaxy exhibits a non-negligible degree of disturbance, which is consistent with the ongoing merging or tidal interaction. The object does not present a clear or obvious disk structure.
