The galaxy presents as a smooth, elongated structure, suggestive of an elliptical morphology. There is a concentration of light towards the center, with a gradual decrease in surface brightness moving outward. No distinct spiral arms or prominent features are discernible within the visible light range. The overall color appears to be relatively uniform, with subtle variations indicating potential differences in stellar populations or dust distribution. The absence of strong color gradients and the smooth texture suggest a relatively old stellar population and a quiescent star formation rate. Based on its shape, it is likely viewed at a high inclination angle. There is no evidence of any ongoing major mergers or significant tidal disturbances.
