The galaxy presents as a smooth, elliptical-shaped structure with a noticeable central bulge. The core exhibits a bright, concentrated luminosity, indicating a high density of stars in that region. Progressing outwards from the core, the luminosity gradually decreases. The outer regions display a diffuse, faint glow with a slight blue tinge, suggesting the presence of younger stars or ongoing star formation activity, though this activity appears subdued. There is no apparent dust lane or spiral arm structure visible. The galaxy exhibits a high degree of symmetry and a generally undisturbed morphology. The axial ratio indicates a moderate flattening, classifying it as an elliptical galaxy, possibly of type E4 or E5 on the Hubble sequence. There's no indication of tidal tails or other features indicative of recent major merger events, although subtle disturbances might be present.
