The galaxy presents an elongated, ellipsoidal morphology. Its color profile leans towards the red end of the spectrum, indicative of an older stellar population. The light is centrally concentrated, with a smooth, diffuse appearance, suggesting a relatively featureless structure without prominent spiral arms or dust lanes. The overall shape is slightly irregular, which may be due to past interactions or ongoing mergers. The surrounding galactic environment appears relatively sparse. High degree of merging fraction suggests a high probability of recent or ongoing galaxy merger.
