The galaxy presents a largely smooth morphology, with minimal discernible features in this image. It appears somewhat elliptical in shape, but is more round than cigar-shaped. The central region exhibits a high concentration of light, indicating a prominent bulge. The color profile suggests a generally older stellar population, with a yellowish-red hue dominating the core and transitioning to slightly bluer colors towards the outer regions. There is no clear evidence of spiral arms, bars, or significant dust lanes. The overall appearance suggests a galaxy undergoing relatively low levels of star formation activity. There are no obvious signs of major mergers or tidal disturbances, although minor asymmetries in the outer halo region cannot be ruled out without further investigation.
