The galaxy presents as a relatively compact structure with a roughly elliptical morphology. Its core appears to be composed of older stellar populations, exhibiting a yellowish-red hue indicative of evolved stars.  There is a faint hint of disk-like structure but it appears dominated by an ellipsoidal shape. There is no obvious spiral arm structure or prominent dust lanes visible. Star formation rate is low, which aligns with the galaxy's color and morphology. The galaxy does not show evidence of any ongoing major merger events or tidal disturbances.  The overall appearance is consistent with a mature galaxy undergoing passive evolution.
