The galaxy presents an elongated, ellipsoidal morphology, suggestive of a spheroid-dominated system. Its overall color profile indicates a population of older stars. The central region appears brighter and more concentrated, exhibiting a yellowish hue, likely indicative of a high density of evolved stars. The outer regions of the galaxy appear fainter, gradually fading into the background sky, but there is also evidence of red color and small pockets of bluer light near the edges of the galaxy, perhaps showing slight star formation. There is no discernible spiral arm structure or distinct dust lanes visible in this image. There appears to be no significant interaction with other galaxies and is not exhibiting clear signs of ongoing major merger events.
