The galaxy presents a generally smooth morphology, with a spheroidal shape. The color profile suggests an older stellar population, with a concentration of light toward the redder end of the spectrum in the galactic center. There is a suggestion of some bluer light in the outer regions, possibly indicative of a small amount of ongoing star formation, although this is not pronounced. No distinct spiral arms or bar structures are discernible. There are a few very faint extensions of light, but otherwise the outer edges of the galaxy fade smoothly into the background sky. There is no clear sign of any active galactic nucleus or strong dust lanes. Overall, the galaxy seems to be a relatively relaxed system without any obvious signs of recent major mergers or interactions.
