The galaxy appears to be a relatively smooth, elliptical or lenticular system, viewed at an oblique angle. The central bulge exhibits a yellowish-white hue, indicating a population of older, evolved stars. A subtle disk is visible, displaying a faint bluish tint which suggests the presence of some younger stars or regions of ongoing star formation, though it is not the dominant characteristic. The overall morphology is generally undisturbed with only a hint of minor asymmetry or disturbance. It does not show any obvious signs of a major ongoing merger or tidal interactions. The galaxy has an elongated shape, appearing to be somewhat cigar-shaped.
