The galaxy appears to be an elliptical galaxy, presenting with a smooth, generally featureless morphology. There is a central, concentrated bulge region exhibiting a yellowish-orange hue, suggesting an older stellar population. This core is surrounded by a more diffuse halo of light, fading into the background sky. The overall shape is roughly round, with minimal deviations from a perfect circle. There is no evidence of spiral arms or a prominent disk structure, nor are there any signs of ongoing major merger activity. A subtle bluish tint is visible in the outer regions of the galaxy, possibly indicating some presence of younger, bluer stars, although the overall stellar population appears dominated by older stars. There is a small indication of minor disturbance or some form of tidal interaction. 
