The galaxy presents as a centrally concentrated object. The core region is characterized by a high luminosity with a pale color profile.

The morphology shows an intermediate galaxy with a central bulge. However, there are some features of potential disturbances in the outskirts of the galaxy, indicating a possible interaction with other objects.

The presence of a blue tone within the galaxy suggests ongoing star formation, though it appears relatively subdued in comparison to what is observed in blue galaxies with high star formation rates. Overall, it seems to be a system that is actively evolving and potentially undergoing changes to its structure through interactions.
