The galaxy presents as a concentrated, ellipsoidal structure. A dominant central bulge is apparent, exhibiting a smooth, fairly uniform luminosity profile that decreases gradually with radial distance. The overall color is yellowish-orange, suggesting an older stellar population with a relatively low rate of ongoing star formation. No distinct spiral arms or dust lanes are discernible in this image. The overall shape approximates a rounded spheroid. There is no visible evidence of any current or recent major merger activity. Faint asymmetric extensions are present in the halo.
