The galaxy appears to be an elliptical galaxy, observed at an inclination nearing edge-on. The overall shape is elongated, suggesting a cigar-like morphology. The central bulge is prominent, exhibiting a yellowish hue, which may indicate an older stellar population. The outer regions of the galaxy display a bluer color, possibly signifying the presence of younger stars or ongoing star formation. There are no readily apparent spiral arm structures or significant dust lanes visible. The galaxy appears relatively smooth and lacks evidence of major disturbances or mergers, though there are some minor irregularities that may suggest a past interaction.
