The galaxy presents as a moderately bright, relatively compact object. Its morphology appears generally smooth with a bright central bulge, showing a slightly elongated shape. There appears to be a faint disk structure surrounding the central bulge. The object's color profile suggests a higher concentration of blue light in the outer regions of the disk, potentially indicating ongoing or recent star formation. In the central region of the bulge, a yellowish color is observed, suggesting the presence of an older stellar population. Evidence of minor disturbances is present, indicating a possible ongoing or past interaction with a smaller galaxy. The galaxy does not seem to have a distinct spiral arm structure.
