The galaxy presents as a single, relatively smooth object with a concentrated central region. The light profile appears centrally peaked, diminishing gradually outwards. Its overall shape is broadly elliptical, showing a slight deviation from perfect roundness, leaning towards a somewhat more lenticular form. Faint color gradients are visible; the central region shows a yellowish hue, potentially indicating an older stellar population, while the outer regions exhibit a bluer tint. This suggests a population with a greater percentage of younger, hotter stars in the outer regions. There is no clear indication of spiral arms, strong dust lanes, or any major disturbances in the galactic structure, though some minor asymmetry cannot be ruled out. The galaxy appears relatively isolated with no other nearby objects in the immediate vicinity to suggest any ongoing or recent interactions.
