The observed galaxy appears as an elliptical or lenticular system, exhibiting a generally smooth, centrally concentrated morphology. Its light profile is dominated by a bulge-like component, with a radial distribution that fades gradually. The overall shape is somewhat flattened, with an apparent ellipticity that suggests a degree of intrinsic rotation. There are no prominent spiral arms or distinct dust lanes visible, indicating a relatively quiescent state. Faint color gradients are observable, trending towards redder hues in the galaxy's core and bluer tints in the outer regions. This may reflect a higher concentration of older stellar populations towards the center and a more recent star formation history in the periphery. Overall, the galaxy exhibits a fairly regular structure, with no obvious signs of major mergers or strong tidal interactions.
