The galaxy presents an elongated, cigar-shaped morphology, indicative of an elliptical or lenticular type. There is a smooth, diffuse glow, with a slightly brighter central region. Hints of a disk may be present but are not well defined, the overall structure appears relatively undisturbed, without prominent tidal features or obvious signs of a major merger event. The color gradient suggests a population of older stars, possibly with ongoing, albeit limited, star formation activity. There are very slight variations in the colour, however, the galaxy presents a primarily red and yellow hue, with slight green tones, indicating the presence of a population of young stars with redder, older population.