The galaxy presents as an elliptical morphology, with a smooth, concentrated light profile. The central region displays a brighter, yellowish hue, suggesting an older stellar population. The galaxy appears moderately elongated, transitioning from a round shape to a slightly cigar-like appearance. There is no clear evidence of spiral arms or significant dust lanes. Faint, diffuse light extends outward from the core, gradually fading into the background. No major distortions or signs of ongoing mergers are readily apparent, although there might be some slight asymmetry or a minor disturbance present. Overall, the galaxy gives the visual impression of a relatively quiescent, evolved system.
