The galaxy presents as a relatively compact object with a smooth, elliptical morphology. There is a defined central bulge exhibiting a concentrated brightness. Around the bulge, there is a distinct ring-like structure or possible spiral arms. These structures are visible due to areas of intense star formation, evidenced by their blue color. Redder hues indicate older stellar populations within the galaxy. The overall structure suggests a galaxy that may be transitioning, possessing features of both spiral and elliptical galaxies. There is no significant evidence of ongoing major mergers, but the possibility of minor disturbances or past interactions cannot be ruled out based on the slightly irregular appearance of the galaxy. The estimated size suggests a galaxy of considerable scale. Overall, it appears to be a relatively evolved galaxy with hints of continued, though potentially low, star formation activity.
