The galaxy presents an elliptical morphology, appearing smooth and relatively featureless. It exhibits a cigar-like shape, elongated along its major axis. The central region displays a concentrated, brighter luminosity, suggesting a dense stellar population. Fainter, diffuse light extends outward from the core, gradually diminishing in intensity. There is a hint of possible dust lanes or substructure within the disk but due to the image quality and small apparent size, it is hard to make an exact estimate. I see no obvious signs of ongoing mergers or major tidal disturbances.
