The galaxy presents as a centrally concentrated object, with a smooth, elliptical morphology dominating the visual appearance. It appears somewhat elongated in shape. There are no obvious spiral arm structures or prominent dust lanes visible. The color profile suggests a population of older stars, with a reddish hue throughout the galaxy body. There is no evidence of a strong, actively star-forming population. Indications are that the galaxy is not undergoing any major merging events or strong tidal interactions with other galaxies. Some degree of disturbance might be happening, but it is not strong enough to say for sure.
