The galaxy presents a primarily smooth and concentrated appearance, indicative of an elliptical morphology or a spiral galaxy viewed at a high inclination. The central region exhibits a bright, yellowish-orange hue, suggesting an older stellar population dominated by red giant stars and a lack of significant ongoing star formation. The galaxy appears elongated, displaying a moderate degree of ellipticity. Faint, diffuse extensions are observed, though no distinct spiral arm structures or prominent dust lanes are discernible in this image. Overall, this galaxy appears relatively undisturbed, showing no strong evidence of recent mergers or tidal interactions.
