The galaxy presents a flattened, elliptical morphology with a prominent central bulge. The bulge exhibits a smooth, yellow-white color profile, indicative of an older stellar population. Fainter spiral arm structures are suspected but not clearly defined, possibly due to the galaxy's inclination. The color shifts towards redder hues in the outer regions of the galaxy, suggesting the presence of dust lanes or a slightly older stellar population compared to the bulge. The overall structure does not show signs of significant tidal disturbances or major merging activity, but there are hints of some minor disturbance. The galaxy has a cigar-shaped morphology.
