The galaxy presents a largely smooth, elliptical morphology. It exhibits a moderate degree of roundness, appearing neither perfectly spherical nor highly elongated. The light distribution is relatively even across the galaxy, with no prominent spiral arms or bar structures visible. There is a slight concentration of light towards the center of the galaxy, suggesting the presence of a galactic nucleus, but it does not appear to be particularly active. The galaxy appears to be a quiescent system, with a lower rate of star formation activity. The overall color of the galaxy appears reddish, indicating a stellar population dominated by older, cooler stars, although there is some evidence of bluer light. There is no significant evidence of tidal tails or other morphological distortions to indicate that it is currently undergoing any major merger activity.
