The galaxy presents a generally smooth, elliptical morphology. It is primarily round in shape, with a very slight elongation. There is no discernible spiral arm structure or prominent dust lanes. The galaxy displays a fairly even light distribution, suggesting a well-mixed stellar population. There is a faint hint of a brighter central region, indicative of a possible galactic nucleus. There are no visible signs of tidal tails, merging events, or major disturbances in its structure. The color appears to be generally redder, suggesting an older stellar population and lower ongoing star formation. Overall, the galaxy appears to be a relatively quiescent, evolved system.
