The galaxy presents a somewhat flattened, elliptical morphology, viewed nearly edge-on. A central bulge appears prominent, exhibiting a brighter, more concentrated luminosity distribution. Extending outwards from the central bulge is a disk-like structure. The disk exhibits a relatively smooth texture with minimal apparent substructure, indicating a lack of well-defined spiral arms. The color gradient suggests a stellar population that is somewhat evolved, with a higher concentration of older stars in the central regions and disk. There is a hint of possible disturbance. The galaxy does not exhibit signs of a high star formation rate or significant dust lanes within the resolution of this image.
