The galaxy appears to be a relatively smooth, elliptical type system. It presents a cigar-shaped morphology, elongated along its major axis. The color profile suggests an older stellar population dominating the light output, exhibiting a yellowish-red hue. There is little evidence of active star formation from the image. There are no clear spiral arm structures or dust lanes visible, contributing to the overall smooth appearance. There is no obvious central bulge, and no indications of any major mergers or tidal disturbances. The galaxy appears relatively isolated and undisturbed, possibly evolving passively.
