The galaxy appears to be part of an interacting system, exhibiting signs of gravitational disturbance and possible merging activity. It has a generally smooth appearance, with a somewhat elongated shape. The color suggests a relatively older stellar population. The light distribution transitions smoothly from the center outward, indicating a lack of distinct spiral arms. There is evidence of tidal tails or extended structures, suggesting ongoing or recent interaction with another galaxy. It appears that the center is compact, but some disruption is present around the edges. The galaxy is somewhat compact with no clearly defined edges.
