The galaxy presents as a lenticular or early-type spiral, though classification is somewhat ambiguous due to the image quality and the galaxy's distance. The galaxy exhibits a notable degree of central concentration, appearing brightest towards the core and fading gradually outwards.

The shape is largely elliptical. There is no prominent disk structure visible. There is faint evidence of a very weak spiral arm.

The galaxy's color is yellowish-orange, indicative of an older stellar population with a lower rate of star formation. There are no prominent HII regions or blue stars visible.

Overall, the galaxy appears to be a relatively massive system. Based on its morphology and color, it is likely a galaxy with a significant population of older stars and a lower rate of current star formation activity.
