The galaxy exhibits a complex morphology, possibly indicative of an ongoing or recent interaction. A dominant, relatively smooth component is visible, appearing somewhat elliptical in shape. This central structure displays a yellow-red hue, suggesting an older stellar population. Extending from this central region is a fainter, more diffuse structure that appears elongated and disrupted. This feature exhibits a bluer color, hinting at the presence of younger stars. The galaxy may be undergoing a minor merger or exhibiting tidal features as a result of gravitational interaction, possibly with two other objects nearby that seem to be connected by faint strands. The color of the main object is indicative of a moderate mass galaxy with a fairly low rate of star formation.
