The galaxy presents an overall elliptical morphology with a smooth light distribution, suggesting a relatively evolved system. There is a subtle color gradient, with the central region exhibiting a slightly yellower hue compared to the bluer, extended outskirts. This color variation is consistent with an older stellar population concentrated in the core, with younger, bluer stars contributing to the outer regions. There is no strong evidence of spiral arm structures or significant dust lanes. The galaxy appears relatively undisturbed, with no obvious signs of recent major merger events. However, there is a faint, diffuse tidal feature extending from one side of the galaxy, possibly indicative of a minor interaction or accretion event in the past. The galaxy appears moderately luminous.
