The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth and concentrated light distribution. The central region presents a significantly higher surface brightness, gradually decreasing towards the outer regions. The isophotes are elongated, suggesting a deviation from a perfectly circular shape, trending towards a cigar-like appearance. There's no clear evidence of spiral arms or a distinct disk structure. Faint color gradients may exist, possibly indicating variations in stellar populations or dust content across the galaxy. The galaxy does not appear to be undergoing any major merging activity, although subtle irregularities could hint at minor disturbances. The overall morphology suggests an older stellar population and relatively quiescent star formation activity.
