The galaxy presents a generally smooth morphology, with a concentrated central bulge. The light distribution suggests a roughly elliptical shape when taking the whole picture into account. The galaxy appears to be undergoing a merging event or tidal interaction, as evidenced by asymmetrical features and faint extensions or distortions in its outer regions, suggestive of a merger remnant. The color profile indicates the presence of an older stellar population, mainly in the central regions, while the overall reddish hue indicates significant dust content. The faint bluer regions suggest areas of ongoing or recent star formation, while the central bright regions appear to show evidence of high stellar density.
