The galaxy presents as a relatively smooth, disk-like structure with an elliptical morphology. The galaxy's core appears concentrated and exhibits a yellowish-orange hue, suggesting an older stellar population. Moving outward from the core, a gradual shift to a greenish tint is observed, potentially indicating the presence of younger stars or ionized gas. The overall shape suggests a possible disk galaxy, but the lack of defined spiral arms makes it difficult to definitively classify. There are no prominent signs of recent major mergers or significant tidal disturbances, though subtle irregularities in the outer regions could indicate minor interactions. The galaxy displays a subtle elongation, appearing more "in-between" round and cigar-shaped.
