The galaxy presents an overall elliptical morphology, elongated along its major axis, appearing cigar-shaped. A central bulge region is clearly visible, exhibiting a concentrated, yellowish-white hue, suggesting a population of older stars. Surrounding the central bulge, a fainter, more diffuse disk is observed. This disk exhibits subtle color gradients, transitioning from a slightly bluish tinge in the outer regions to a more neutral color closer to the bulge. The disk appears relatively smooth, lacking prominent spiral arm structures or distinct dust lanes. There is no obvious evidence of active galactic nuclei or significant starburst activity based on visual inspection alone. The galaxy appears to be a relatively isolated system, with no signs of major tidal interactions or mergers readily apparent, although some minor disturbance cannot be fully ruled out at this resolution.
