The galaxy presents a generally smooth, elliptical morphology. The central region displays a concentrated luminosity profile, exhibiting a bright, yellowish-white hue. Moving outwards from the core, the light gradually diminishes. The overall shape is close to round, showing minimal apparent distortion. There is no clear indication of spiral arms or a prominent disk structure. Faint, diffuse bluer tones can be observed in the outer regions, suggesting some level of ongoing star formation, though not at a high rate. No significant merger events or tidal disturbances are apparent.
