The galaxy presents as a late-type spiral, seen nearly edge-on. It possesses a prominent, centrally located bulge that appears relatively smooth and concentrated. The disk component is easily discernable, but without prominent spiral arm structure visible. The light distribution suggests a flattened spheroid shape, with a higher concentration of older stellar populations in the bulge region indicated by the color. The dust lane is visible, and there is a possible indication of faint tidal features. These disturbances are indicative of a galaxy that is potentially undergoing minor interactions with another galaxy, or has undergone one in the past. Overall, the galaxy displays characteristics consistent with an evolved spiral system, potentially experiencing some environmental influence.
