The galaxy exhibits an elongated, cigar-shaped morphology, indicative of an elliptical galaxy. Its central region displays a concentrated, yellowish hue, suggesting a population of older stars. The outer regions appear fainter and bluer, possibly due to the presence of a younger stellar population or a small amount of ongoing star formation. There's a smooth gradient in luminosity from the core outwards. There are no visible spiral arms or distinct dust lanes. It is a relatively isolated galaxy, showing no apparent signs of ongoing merger activity. The major axis is oriented at an angle. Overall, it appears to be a fairly typical, relatively low-mass elliptical galaxy.
