The galaxy presents as a somewhat diffuse object with a moderate central concentration of light. A slightly elliptical morphology is suspected, although the apparent fuzziness makes precise determination difficult. The color profile suggests a mix of stellar populations, exhibiting a subtle shift from a potentially older, redder core to bluer outer regions, possibly indicating ongoing or recent star formation within the disk. There are indications of minor disturbances in the structure, maybe caused by tidal interactions or other past merger events. A small portion of the galaxy seems to be disrupted, or merging. The galaxy displays moderate star formation, which means its color is neither very blue nor very red.
