The galaxy presents a generally smooth morphology, suggestive of an elliptical or lenticular classification. The light distribution appears centrally concentrated, with a noticeable elongation along one axis, exhibiting a cigar-shaped appearance. There is a small but noticeable disturbance to one side of the galaxy, this could be evidence of a minor interaction or a faint tidal feature. Color gradients suggest a population of older stars dominate the galaxy’s stellar content, with a central yellowish or reddish hue. The overall structure does not show strong spiral arm features or significant dust lanes, further supporting the smooth morphology.
