The galaxy presents as an elliptical structure, exhibiting a high degree of smoothness. It is nearly circular in appearance, showing minimal deviation from a perfectly rounded shape. The core of the galaxy is significantly brighter and appears more yellow than its surrounding regions. There is a relatively smooth transition of light intensity from the core to the outer edges, suggesting a lack of prominent spiral arms or distinct features within the galaxy disk. The overall color profile indicates an older stellar population, with a diminished presence of dust lanes or active star-forming regions. There is no indication of significant tidal disturbances or ongoing major mergers. The galaxy appears to be a relatively isolated system, showing no evidence of nearby companion galaxies strongly influencing its morphology.
