The galaxy presents as a single, largely homogenous structure, likely a spheroid. Its color is predominantly yellow to orange, indicative of an older stellar population and a low rate of current star formation. There is a concentration of luminosity toward the center suggesting a bulge. No distinct spiral arms or features are apparent, lending credence to its possible classification as an elliptical galaxy, although the outer regions are not well-resolved in this image. Any assessment of tidal features is not possible given the image quality. There is no obvious dust lane structure. The apparent smoothness suggests an older stellar population with well-mixed components. The galaxy does not show any indication of a major merger or strong tidal interaction.
