The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that is yellowish-white in color, suggesting an older stellar population. The surrounding disk appears less pronounced, with a slightly bluer hue indicating some ongoing star formation, although at a relatively low rate. The galaxy's shape is more in between elliptical and disk-shaped, appearing to be less rounded or particularly cigar-shaped. There is no strong evidence of major mergers or significant tidal disturbances affecting the galaxy's overall structure. Overall, the galaxy seems relatively isolated and unperturbed.
