The galaxy presents as a flattened, elliptical form, with a pronounced central bulge. The light distribution appears relatively smooth and concentrated, suggesting an older stellar population dominates. There are some faint disks, though no distinct spiral arm structure is visible in this image. The major axis of the ellipse is more extended than the minor axis, resulting in a cigar-like appearance. There is no obvious presence of significant tidal disturbances or ongoing major merging activity. Overall, the galaxy's morphology indicates a relatively quiescent state, possibly with a low star formation rate. The central region exhibits a brighter, more yellowish hue, while the outer regions appear slightly bluer, indicating potential differences in stellar populations.