The galaxy exhibits an overall elliptical morphology, appearing elongated with a high degree of central concentration. The light distribution is smooth, suggesting an older stellar population. The central region displays a yellowish hue, which could indicate the presence of older stars or dust absorption. Fainter extensions of light are visible along the major axis, with some asymmetry in the outskirts. There are no prominent spiral arms or significant dust lanes visible. There may be some sign of a minor disturbance, however, the overall structure appears relatively undisturbed. The visible diameter of the galaxy is estimated to be approximately 6 kpc. There is some evidence of ongoing, though low, star formation. The estimated mass suggests this is a massive galaxy.
