The galaxy presents as a relatively compact, elliptical or spheroidal structure. It exhibits a smooth, diffuse light distribution, lacking prominent spiral arms or a distinct central bulge. There is a noticeable blue hue throughout the galaxy, indicating the presence of a moderate population of young, hot stars, suggesting ongoing or recent star formation activity. Its round morphology is indicative of a dynamically relaxed system, and the color profile is suggestive of a late-type system with moderate amounts of dust obscuration. There are no signs of tidal tails, strong gravitational lensing, or significant morphological disturbances, implying the galaxy is not currently undergoing a major merger or strong interaction with another galaxy.
