The galaxy presents as a concentrated central region with a notable degree of smoothness. There is likely a faint disk or arm-like structure, although the smoothness is dominant and well-defined. The galaxy's shape appears close to round, rather than elongated, and the colors are dominated by a redder hue. The galaxy exhibits signs of ongoing or recent interaction, showing signs of a merger or disturbance, or multiple merging events. The colors are not strongly indicative of active star formation, instead leaning towards an older stellar population.
