The galaxy presents as a generally smooth, elliptical-like object. Its shape is elongated, appearing cigar-shaped rather than perfectly round. There is a slight color gradient observed, with a subtle redder hue towards the central region, potentially indicating an older stellar population concentrated there. Hints of bluer colors exist at the edges of the galaxy. No prominent spiral arms or obvious dust lanes are observed. The galaxy does not appear to be undergoing any major mergers or tidal disturbances based on its overall structure, though subtle asymmetries are present in its outer regions.
