The galaxy presents a generally elliptical morphology. The light distribution appears relatively smooth and centrally concentrated, indicative of a spheroid-dominated system. The galaxy exhibits a subtle elongation, with a notable cigar shape, deviating from a perfectly circular form. There is no obvious spiral arm structure or prominent dust lanes visible. Color gradients across the galaxy appear subtle, with a slightly bluer hue in the central regions. There is no apparent significant ongoing merger activity or major tidal disturbance. Overall, the galaxy appears to be a relatively undisturbed system.
