The galaxy presents as a flattened disk, appearing elongated in shape with a noticeable major axis. Its color gradient suggests a relatively older stellar population, with light concentrated toward the redder end of the spectrum. The central region of the galaxy appears brighter and more concentrated. There is a slight warp or irregularity to the disk structure. The galaxy exhibits an axial ratio of approximately 0.4, indicating a significantly inclined orientation with respect to our line of sight. The light distribution follows a Sersic profile. There are indications of minor disturbances, possibly resulting from past interactions.
