The galaxy appears to be a relatively smooth, elliptical system. Its overall morphology is round with no obvious signs of a disk component or spiral arms. The light is concentrated towards the center with a bright, yellowish core, suggesting an older stellar population dominates the central region. There is a gradual fading of light intensity outward from the core. Fainter, bluer hues in the outer regions may indicate the presence of younger stars, but these features are not prominent. No distinct dust lanes or tidal features are visible, implying a dynamically relaxed state. The galaxy appears undisturbed, with no major signs of recent or ongoing mergers.
