The galaxy presents as a centrally concentrated object, characterized by a smooth, elliptical morphology. Its overall color profile leans toward the red end of the spectrum, suggesting an older stellar population. There is no discernable disk component or spiral arm structure. Visual inspection indicates a high degree of central concentration, with a gradual decrease in surface brightness moving outwards from the core. No evidence of ongoing major merging activity or tidal disturbances are apparent. The galaxy appears relatively isolated within the observed field. Given the red color and lack of distinct features, the galaxy is likely a relatively quiescent system with low rates of star formation.
