The galaxy presents as a well-defined elliptical structure with a notably smooth morphology. Its central bulge is prominent, exhibiting a concentrated luminosity profile that graduates into a fainter, more diffuse halo. The galaxy's orientation is oblique relative to our line of sight, indicating a significant inclination. There are subtle color variations visible; the central bulge displays a yellowish-red hue, possibly indicating an older stellar population, while the outer regions exhibit a bluer tint, suggesting the presence of younger stars. No distinct spiral arm structures or prominent dust lanes are apparent. There are no visible signs of recent major merger activity or tidal disturbances.
