The galaxy presents as a relatively smooth, elliptical-type structure, exhibiting a concentrated, luminous core. The overall shape is more akin to an ellipse than a disk galaxy. There is a slight asymmetry to the object, but no clear indication of spiral arms or strong tidal features. The light is primarily yellowish-orange, indicative of an older stellar population dominating the light output. There is a faint, extended halo or envelope surrounding the central region, suggesting a more diffuse distribution of stars at larger radii. No distinct dust lanes or prominent star-forming regions are readily apparent. The galaxy appears relatively isolated, without obvious signs of ongoing merger activity or significant interaction with companion galaxies.
