The galaxy presents as a moderately luminous object with an apparent elliptical morphology. The central region exhibits a bright, concentrated core that gradually fades into a diffuse halo. The primary color of the core appears to be yellowish-orange, suggesting an older stellar population.  A subtle, bluer hue can be discerned in the outer regions of the galaxy, particularly towards the edges of the halo, possibly indicating the presence of younger, hotter stars or ongoing star formation at a low rate. There is a potential minor visual disturbance in the galaxy's morphology, such as a slight asymmetry or tidal feature, hinting at a possible past or ongoing interaction with a smaller companion galaxy or intergalactic medium. A separate, less luminous object is present in the field of view that is potentially interacting with the galaxy.