The galaxy presents as a relatively small, elongated structure with a high degree of smoothness in its overall appearance. It exhibits a slightly cigar-shaped morphology, suggestive of an elliptical galaxy. No prominent spiral arms or distinct features indicative of active star formation are readily discernible from the image. There is a subtle color gradient visible, with the central region appearing marginally more luminous and having a slightly redder hue than the outer regions, possibly indicating a higher concentration of older stellar populations in the galactic nucleus. The overall structure suggests a relaxed system, potentially exhibiting signs of a more evolved galactic form with a low rate of star formation. There do not appear to be any major tidal disturbances or indications of ongoing mergers with other galaxies. 
