The galaxy presents as a somewhat diffuse, centrally concentrated object with a hint of a spiral structure. The core region exhibits a brighter, more condensed luminosity, suggestive of a central bulge. While the overall shape is largely smooth, there is a noticeable distortion or plume extending from the lower portion, indicating a possible interaction or merger event. The color appears blue-shifted, possibly indicating active star formation. The spiral arms, if present, are not well-defined, but the slight asymmetry and extended feature point to a galaxy undergoing some form of gravitational disturbance, potentially due to a past or ongoing interaction with another galaxy.
