The galaxy presents a roughly elliptical morphology, though the core is not perfectly spherical. The central region exhibits a concentrated, bright core indicating a significant stellar density. Around the core, a fainter, more diffuse halo is visible, suggesting a transition to a lower stellar density at greater radii.

The light distribution appears somewhat uneven, and there are possible signs of minor disturbances within the galaxy's structure. Faint extensions or tidal features may be present, hinting at past or ongoing gravitational interactions with other galaxies. The galaxy's color profile suggests a relatively old stellar population.
