The galaxy presents as a slightly elongated, lenticular structure. There's a central bulge of moderate intensity, appearing smooth and diffuse, with a yellow to white hue, suggesting an older stellar population. The disk component exhibits a faint, dusty red band, which may indicate some ongoing, yet minimal, star formation, or simply older stars. The galaxy's overall structure appears relatively undisturbed, with no obvious signs of a major ongoing merger or tidal disruption. A subtle blueish tinge hints at the presence of younger stars. The galaxy appears to be reasonably well defined, the edges are diffuse, possibly due to its distance. It is an isolated galaxy, not part of a larger cluster or interacting with nearby galaxies. Overall, this appears to be a fairly massive galaxy, transitioning from active star formation to a more quiescent phase.
