The galaxy appears as a moderately bright object exhibiting a slightly elongated morphology, indicating a shape that deviates from being perfectly circular. The light distribution suggests a central bulge with a surrounding disk component.

There is evidence of internal structure, though not sharply defined. Faint, diffuse features may represent spiral arms or tidal tails. The color gradient indicates a higher concentration of older stars towards the galactic center, which may have diminished star formation. The outer regions present a bluer hue suggesting ongoing star formation. 

There appears to be some distortion in the galaxy's structure suggesting possible past or ongoing interactions with another galaxy.
