The galaxy appears as a relatively small, compact object. It exhibits a generally smooth morphology with a largely featureless disk. The color profile shows a gradient, appearing bluer at the core and gradually becoming redder towards the outer regions. This color gradient suggests potential differences in stellar populations, with younger, hotter stars possibly dominating the central regions and older, cooler stars prevalent in the outskirts. There is no obvious spiral structure or bar feature visible, suggesting that it is possibly an elliptical or lenticular galaxy. There may be some minor gravitational disturbance.
