The galaxy presents a largely elliptical morphology. Its light profile is relatively smooth, with no apparent spiral arm structures or strong dust lane features visible at this resolution. The color index, inferred from the image's color composition, suggests a relatively evolved stellar population, tending towards redder hues in the galaxy's core and diminishing outward. The galaxy appears somewhat compact, exhibiting a moderately high degree of central concentration. There is a subtle hint of asymmetry, but it is difficult to determine if this is due to an ongoing minor interaction or internal structures. There is no indication of major mergers or tidal tails in the current observation. Based on these observations, it seems to be a fairly massive galaxy with a modest ongoing star formation rate.
