The galaxy presents an elliptical morphology, appearing largely smooth and spheroidal. The light distribution is concentrated towards the center, exhibiting a strong central bulge. A slight asymmetry is detected within the galactic profile, possibly due to ongoing interactions. Some faint redder regions are present, indicating older stellar populations. This galaxy appears to be a relatively evolved system, with minimal evidence of recent star formation. Faint light is dispersed throughout the entire galaxy, creating a subtle halo.
