The galaxy presents an elliptical morphology, exhibiting a smooth, largely featureless structure. Its overall shape is elongated, appearing cigar-shaped. The central region displays a concentrated luminosity, suggesting a prominent galactic nucleus. The light profile gradually fades outwards from the core, showing a diffuse halo. There's a subtle color gradient, shifting from a yellowish-white core to slightly redder hues in the outer regions, indicative of potential variations in stellar populations and dust content. No distinct spiral arms, bars, or tidal features are discernible within the observational data. The galaxy doesn't present any obvious signs of ongoing major merger activity or significant morphological disturbance.
