The galaxy exhibits a moderately disturbed morphology, possibly indicative of an ongoing or recent merger event. The overall shape appears somewhat irregular and distorted, lacking a clear spiral arm structure or a well-defined elliptical form. The light distribution suggests a central concentration of luminosity with a more diffuse and less structured outer region. The observed color gradient appears to have a bluer core region surrounded by a redder envelope. The galaxy exhibits an estimated effective radius of approximately 5 kiloparsecs, suggesting an intermediate size within the galactic population. There is a faint suggestion of tidal tails or extended features, but these are not sharply defined. The integrated light suggests moderate star formation activity.
