This galaxy presents a largely elliptical morphology, appearing primarily smooth in structure. The central region exhibits a concentrated luminosity gradient, suggesting a prominent galactic nucleus. Extending outwards, the light distribution gradually decreases in intensity, with a generally round appearance. There is a subtle bluish tint around the central part, which could denote the presence of some younger stellar populations. There is no strong evidence of significant tidal disturbances or ongoing major merger activity based on its morphology.
