The galaxy presents as a mostly smooth structure with hints of features suggestive of a disk. The color distribution indicates a central region with a dominant bluish hue, potentially indicating active star formation, grading into a more redish and elongated shape. The elongated form is somewhat cigar shaped. The overall light distribution is moderately concentrated, suggesting neither a pure elliptical nor a highly structured spiral. There may be some level of galactic interaction or disturbance present in the structure.
