The galaxy appears to be an elliptical galaxy, exhibiting a smooth, featureless morphology. Its overall shape is elongated, appearing as a somewhat flattened spheroid or a cigar shape. The light distribution suggests a central bulge that is bright and concentrated, becoming gradually fainter towards the outer edges. The color profile shows a predominantly redder hue, particularly in the central regions, which could indicate an older stellar population. There is a slight color gradient, with the outer edges of the galaxy exhibiting a subtle shift toward bluer wavelengths, suggesting the presence of some younger stars or low levels of recent star formation. There are no apparent signs of significant dust lanes, spiral arms, or major disturbances, supporting the classification of an elliptical galaxy. No close companions or indications of merging are visible in this image, and the galaxy appears to be relatively isolated.
