The galaxy presents as a somewhat elongated, cigar-shaped structure. It appears relatively smooth in texture, with no distinct spiral arms or bar visible. The central region exhibits a higher concentration of light, suggesting a prominent bulge or nucleus. The color gradient transitions from a yellow-orange core to a slightly redder outer halo. This color profile may indicate an older stellar population dominating the central regions and possibly ongoing, but diminished, star formation in the outer parts. There are some suggestions of minor disturbance in the outer parts of the galaxy. Overall, the galaxy’s morphology is suggestive of an elliptical type or a lenticular galaxy with a notable spheroidal component.
