The galaxy appears as a centrally concentrated object, exhibiting a bright, somewhat irregular core region. The light profile suggests a relatively smooth overall structure, but there are noticeable deviations from perfect ellipticity in the outer regions. A faint and diffuse halo surrounds the core. There may be a tidal tail to the left of the image, however this is highly uncertain. Some indication of minor disturbances in the morphology is present, though the dominant impression is of a relatively undisturbed system. This suggests a possible ongoing or recent minor interaction event. There are some indications that the center of the galaxy is slightly offset, supporting the possibility of an interaction. The galaxy displays a bluish hue in its core and inner regions, which may indicate the presence of younger, hotter stellar populations or active star formation.
