The galaxy presents as an elliptical morphology, with an elongated, cigar-shaped appearance. The central bulge is prominent and exhibits a yellowish-orange hue, suggesting an older stellar population with a lower rate of star formation. Moving outward from the core, the color shifts toward a slightly bluer tone in the outer regions, perhaps indicating a small population of younger, hotter stars, or more likely a lower concentration of dust. The overall structure appears relatively smooth, without any obvious spiral arms or significant dust lanes. There is no visually apparent interaction or merging event currently underway, though subtle distortions may suggest a past interaction. The galaxy appears relatively isolated in its immediate vicinity. The redshift suggests a considerable distance, contributing to the somewhat blurred appearance and limiting the detection of finer details.
