The galaxy exhibits an overall elliptical morphology, appearing elongated with a cigar-like shape. The light distribution is relatively smooth, indicating a lack of prominent spiral arms or significant dust lanes. There is some indication of slight disturbances in the structure, potentially hinting at minor interactions or past merger events. The core of the galaxy is more luminous, with its intensity gradually decreasing towards the outer regions. Color gradients suggest a possible variation in stellar populations across the galaxy. Overall, this appears to be a galaxy characterized by evolved stellar populations and quiescent star formation.
