The galaxy presents with a yellowish-white core, exhibiting a moderate degree of central concentration. Its overall shape is elongated, suggesting a possible elliptical or lenticular morphology. The light distribution is relatively smooth, with no distinct spiral arm structures visible, indicating a lack of prominent star-forming regions. There is an apparent companion galaxy in proximity, showing signs of tidal disturbance, possibly indicative of a gravitational interaction or ongoing merger event. Faint extensions or plumes can be seen emanating from the core region, further supporting the possibility of a minor disturbance or past interaction. The galaxy has an estimated size of approximately 7 kpc and appears relatively massive with a moderate star formation rate.
