The galaxy appears as a centrally concentrated object with a generally smooth morphology. There is evidence of a slightly elongated shape. The color profile suggests an older stellar population concentrated in the core, indicated by the yellowish-orange hue. A fainter, more diffuse bluish component is visible in the surrounding regions, possibly indicating some ongoing, albeit low-level, star formation within a disk-like structure. There may be some minor disturbances within the overall structure. No large-scale spiral arms or significant tidal features are readily apparent.
