The galaxy appears to be a relatively smooth, elliptical system, exhibiting a centrally concentrated light profile. Its overall shape approximates a rounded form. The core displays a bright, yellowish-white hue, suggesting an older stellar population with minimal ongoing star formation. Fainter blueish emissions extend from the center of the galaxy, likely indicating the presence of a younger stellar population. There is no evidence of significant dust lanes or spiral arm structures. The galaxy is not obviously interacting with other systems; there is little evidence of tidal tails or other morphological distortions typically associated with mergers. The overall appearance suggests it may be a mature galaxy with a stellar mass of approximately 10^10 solar masses and only mild star formation activity.
