The galaxy appears to be an elliptical galaxy, exhibiting a smooth, diffuse light distribution without distinct spiral arms or a prominent central bulge. It presents an elongated, cigar-like shape. The core region displays a slightly brighter, more concentrated luminosity, gently fading towards the outer edges. The galaxy's color profile suggests an older stellar population, with a redder hue dominating the central regions and a subtle transition to slightly bluer tones in the periphery, which may indicate the presence of younger, star-forming regions in the galaxy's outskirts, though star formation appears to be relatively low. There is no visual evidence of active galactic nuclei activity, such as a bright, point-like source at the center, nor are there any apparent signs of ongoing or recent major mergers, like tidal tails or significant distortions in the galaxy's overall morphology. The galaxy appears relatively undisturbed.
