The galaxy presents as an elliptical or lenticular structure with a smooth overall appearance. The light distribution is concentrated centrally, exhibiting a gradual decrease in intensity towards the outer regions. The galaxy's shape appears elongated, with an axial ratio significantly less than 1, suggesting it is viewed at an oblique angle. No distinct spiral arms or prominent dust lanes are discernible. There may be some evidence of disturbance to the galaxy's morphology. The color profile indicates the presence of a relatively old stellar population.
