The galaxy presents as a lenticular or possibly an elliptical galaxy, displaying a smooth, concentrated luminosity profile. The morphology is elongated, with an axis ratio suggesting a significant degree of flattening. The central bulge region exhibits a brighter, yellower hue, indicating a higher concentration of older stellar populations. The outer regions of the galaxy gradually fade into the background, exhibiting a redder color. No distinct spiral arm structures or prominent dust lanes are discernible. There is no indication of ongoing major merger activity, although there is subtle evidence of a minor asymmetry or disturbance in the outer regions. The galaxy has a low rate of star formation.