This galaxy presents as a relatively smooth, elliptical structure. The core region is bright, indicating a high concentration of stars. Moving outward, the luminosity gradually decreases, transitioning into a faint halo. There is a slight bluing in the core and inner region, which could be caused by ongoing star formation, or it may simply be an artifact of how the image was taken. However, there is a notable absence of distinct spiral arms or prominent dust lanes typically associated with spiral galaxies. The overall symmetrical, rounded shape supports the conclusion that it is likely an elliptical galaxy undergoing minimal tidal interactions or disturbances. There are some very faint, slightly elongated features near the edge of the galaxy that are indicative of very small tidal tails or plumes. These features suggest a past minor interaction with another galaxy.
