The galaxy presents an elongated, cigar-shaped morphology. It displays a relatively smooth texture throughout, indicative of an elliptical galaxy type. The central region appears brighter and more concentrated than the outer edges. A color gradient is observed, with the core showing a yellow-white hue, possibly indicating an older stellar population. Moving towards the periphery, the color shifts to a more red-tinged profile. No distinct spiral arms or prominent dust lanes are visible. There is a subtle distortion in the shape, possibly indicative of tidal interactions with a nearby galaxy or gravitational influences. Signs of any major ongoing merger events are not apparent, though minor disturbances cannot be ruled out.