The galaxy presents as a relatively smooth, elliptical structure, with minimal discernible features such as spiral arms or prominent dust lanes. Its overall morphology suggests an evolved system. The core exhibits a yellowish hue, possibly indicative of an older stellar population, with an apparent absence of significant on-going star formation in that region. A subtle transition to a greenish-blue color is observed in the outer regions of the galaxy, potentially signaling the presence of a younger, hotter stellar population in these areas, although the star formation rate is likely suppressed. The galaxy appears largely undisturbed, lacking any obvious signs of recent merger activity or tidal distortions. Its shape is observed to be an ellipse, with a high level of roundness.
