The galaxy presents as a relatively smooth, elliptical form, elongated along a defined major axis. A central bulge region is clearly visible, exhibiting a brighter, more concentrated luminosity compared to the outer regions. The color profile suggests a dominant population of older stars, with a noticeable redder hue concentrated in the central bulge, transitioning to slightly bluer tones towards the outer regions of the galaxy. There is no apparent spiral arm structure or significant dust lane obscuration evident in this image. The overall morphology indicates a mature system, potentially an elliptical galaxy. There is also a slight curvature that might be a minor disturbance that shows possible signs of a merger event. 
