The galaxy presents an overall elliptical morphology, appearing mostly smooth in structure with no readily discernible spiral arms or bar features. The central region displays a high concentration of light, suggesting a prominent galactic bulge. A gradual decrease in luminosity extends outward from the core, forming a diffuse halo. The color gradient shifts from a yellowish-white in the center to a faint bluish hue at the outer edges. This may indicate a mixed stellar population with older stars dominating the core and younger, bluer stars populating the outer regions where there may be low levels of star formation. The galaxy's apparent shape is slightly elongated, with a ratio of major to minor axes approximately 3:2, classifying it as an elliptical galaxy of type E4 or E5 on the Hubble sequence. The overall morphology is suggestive of a mature galaxy, likely undergoing a period of quiescence. There is no evidence of significant tidal disturbances or ongoing major mergers.
