The galaxy presents as a relatively smooth, elliptical form. Its overall color appears to be a yellowish-orange, which suggests an older stellar population and a lower rate of active star formation. The shape is elongated, appearing cigar-shaped rather than perfectly spherical, indicating some level of flattening or possible rotational influence. There are no obvious signs of major mergers or significant tidal disturbances visible. A slight central bulge is discernable due to the increase in color saturation. Based on the color, there are possible signs of dust absorption, indicating the presence of interstellar matter. Further spectroscopic data would be needed to confirm its composition and age distribution.
