The galaxy presents an overall smooth morphology, exhibiting a slightly elongated, elliptical shape. There's a noticeable color gradient within the galaxy; the central region appears reddish, possibly indicating a population of older stars or dust obscuration. Moving outwards from the center, the color shifts towards greenish hues, which could indicate a population of younger stars or regions of active star formation. Although generally smooth, there appear to be some subtle hints of faint, diffuse features around the main body of the galaxy, suggesting possible tidal interactions or past mergers. The overall structure suggests that it is a fairly massive system, with moderate star formation activity.
