The galaxy presents as a moderately bright object with a relatively compact structure. It appears somewhat amorphous, with no immediately obvious spiral arm structures. The central region exhibits a brighter, more concentrated luminosity, possibly indicating a galactic bulge or active galactic nucleus. There is a slight elongation or asymmetry to the overall shape, hinting at a possible past or ongoing interaction. The color profile suggests a mix of stellar populations; a bluer component is visible, possibly indicating recent star formation, mixed with more yellowish hues typical of older stars. There are subtle features extending outward from the main body of the galaxy, which may be tidal features.
