The galaxy appears to be a relatively smooth, disk-shaped system with an overall elliptical morphology. A slight central bulge is visible, appearing more luminous and concentrated than the surrounding disk. The galaxy exhibits a color gradient, transitioning from a bluer hue in the outer regions, suggestive of younger stellar populations and ongoing star formation, to a yellower hue towards the central bulge, which indicates an older, redder stellar population. The dust lanes are either not visible or extremely faint. While no major disturbances are obvious, there may be a minor interaction occurring that has distorted the light. The galaxy is not perfectly round, exhibiting a slightly elongated shape.
