The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. Its overall shape appears slightly elongated, but not significantly cigar-shaped. The color profile suggests a dominant population of older stars, exhibiting a yellowish hue. There is evidence of some minor internal structures, potentially indicative of a disk component or subtle disturbances within the galaxy. No significant signs of major mergers are discernible, though a possible minor interaction with a smaller galaxy cannot be ruled out based on the image alone. The galaxy shows moderate star formation activity. Overall, it appears to be a mature galaxy, undergoing relatively quiescent evolution.
