The galaxy appears as a centrally concentrated object with a relatively smooth profile. The overall shape is generally round, showing a slight deviation towards an elliptical form. There is no distinct bulge or disk structure readily apparent in the image. The color distribution exhibits a notable red hue, suggesting a stellar population dominated by older, redder stars or significant dust obscuration. No significant tidal features, spiral arms, or signs of active galactic nuclei are discernible from this image. The galaxy appears relatively isolated, with no immediate companion galaxies or indications of ongoing merger activity. Based on its apparent morphology, color, and lack of significant features, this galaxy is likely an elliptical or lenticular type system with a minimal rate of current star formation.
