The galaxy presents an overall elliptical morphology, appearing relatively smooth in structure with no prominent spiral arms visible. The central region exhibits a higher concentration of light, suggesting a well-defined galactic nucleus. The light gradually diminishes towards the outer edges of the galaxy, exhibiting a fuzzy halo. Color gradients are subtle, with a slightly bluer hue in the central region potentially indicating the presence of younger stellar populations, transitioning to redder tones towards the outer regions, possibly due to older, redder stars dominating in these areas. There is some indication of minor disturbance or asymmetry in the galactic disc, although it is not classified as a major merger event. Overall, the galaxy appears to be a relatively undisturbed, moderately sized system with evidence of a mix of stellar populations.
