The galaxy presents a generally smooth morphology with a notable central bulge. The bulge exhibits a yellowish-white hue, suggesting an older stellar population, while the surrounding disk appears somewhat bluer, indicative of ongoing star formation. There may be some evidence of a slight disturbance within the galactic structure, potentially hinting at minor interaction. The galaxy appears as an intermediate ellipse. There is a concentration of light toward the center, and it looks like a lack of spiral arm structure.
