The galaxy presents an elongated, cigar-shaped morphology, suggesting it could be classified as an elliptical galaxy or an edge-on spiral galaxy. The primary body exhibits a relatively smooth appearance, with a gradual increase in luminosity towards the center. The color profile displays a central region of yellowish hues, which may indicate an older stellar population dominating the core.

The galaxy does not display distinct spiral arm structures or prominent dust lanes. There is a hint of redder light at the edges of the object. Overall, the galaxy appears relatively isolated, although it may be interacting with a smaller object nearby. The lack of strong blue light indicates a low rate of recent star formation. The galaxy appears to be a large mass system.
