The galaxy appears as a single, centrally concentrated object, likely an elliptical galaxy due to its smooth morphology and lack of discernible spiral arms or a distinct disk. It exhibits a radial color gradient, with the core region being predominantly yellow, suggesting an older stellar population. The outer regions transition to a redder hue, which could be due to a combination of dust obscuration or an even older, redder stellar population. The galaxy's light is evenly distributed, showing no strong indications of recent major mergers or tidal disturbances. It has a generally round shape, with a slight deviation, but no cigar shape. There are no discernible star-forming regions or features indicative of active star formation. The object appears to be relatively isolated, with no companion galaxies immediately apparent that could suggest an ongoing interaction.
