The galaxy presents as a relatively smooth, elliptical-like structure. Its core is characterized by a concentrated, bright region, exhibiting a yellowish-red hue. The intensity of the light appears to decrease gradually towards the outer edges, creating a diffuse halo around the central core. Faint hints of what may be spiral arm structures can be seen but they are not very pronounced. There are some small blue patches within the diffuse halo region, possibly indicative of star forming regions. The overall morphology suggests a galaxy that is not currently undergoing significant merging or major disturbances.
