This galaxy appears to be a relatively smooth, elliptical system. It exhibits a centrally concentrated luminosity profile, with a bright nucleus that gradually fades into a diffuse halo. The galaxy has a generally round shape, showing very little evidence of strong disturbances in its morphology. It is likely that the stars in the galaxy are largely older, redder stars. There may be some ongoing star formation, but the rate is likely quite low, as there are no strong indicators of the presence of significant populations of young, massive stars in the galaxy's disk. There does not appear to be any recent major merger events or tidal interactions evident in its structure. The overall smooth and symmetrical appearance suggests that this galaxy is a well-mixed, relatively dynamically relaxed system.
