The galaxy presents as a well-defined elliptical morphology. The central region exhibits high luminosity, appearing nearly spherical and concentrated. Moving outward from the core, the luminosity decreases gradually. The outer regions appear smooth with some light, indistinct features. The galaxy shows an overall reddish-yellow hue, likely indicative of an older stellar population and a lower rate of ongoing star formation. There is no prominent disk structure or spiral arm pattern visible. The observed shape suggests a relatively high degree of flattening. No signs of major merger events or significant tidal disturbances are apparent within the immediate vicinity of the galaxy.
