The galaxy appears as a relatively compact object with a bright, concentrated central region. The morphology suggests a predominantly smooth structure, but with subtle deviations from perfect symmetry. There is an indication of a faint extended halo or envelope surrounding the brighter core.

Color gradients are observed, with the central region exhibiting a bluer hue that may indicate ongoing or recent star formation activity. The outer regions appear redder, possibly due to an older stellar population.

Based on the faint asymmetry and the presence of color gradients, there's a marginal possibility of a past minor interaction or merger event, although the galaxy appears largely undisturbed in its present state. Further spectroscopic data is required to measure the stellar populations, kinematics, and any possible active galactic nucleus activity. Higher resolution imaging may be needed to clarify the presence of any faint tidal features or finer structures.
