The galaxy presents as a largely smooth, elliptical morphology. It exhibits a concentrated central bulge that is strongly luminous, indicating a high density of stars in that region. The light appears yellowish-red, suggestive of an older stellar population with a minimal presence of young, blue stars.

The overall shape is generally round. There are no apparent spiral arms or disk-like structures visible. It does not display any significant signs of recent major merger activity or tidal disturbances. The faint extensions around the central region may be indicative of a diffuse halo, but more data would be needed to confirm its properties and extent. There is little evidence of significant ongoing star formation based on the observed color profile.
