The galaxy presents as a relatively smooth, elliptical structure. Its overall shape is elongated, approximating a cigar shape. A bright, concentrated central bulge is apparent, with the light intensity gradually decreasing towards the outer edges of the galaxy. The color profile suggests a higher concentration of older stars, particularly within the central bulge, as indicated by the yellower hue. There are hints of bluer regions in the outer parts, suggesting the presence of younger stars or ongoing star formation, although these features are subtle. No significant signs of spiral arm structures or major disturbances are visible. The overall morphology suggests a galaxy that is either an elliptical or possibly a lenticular galaxy viewed edge-on, with a relatively high stellar mass and a low rate of star formation. There appears to be no active galactic nucleus easily observable in this image.
