The galaxy presents an elliptical morphology, appearing largely smooth and featureless in this image. Its overall shape is elongated, with a cigar-like appearance, suggesting it is not perfectly spherical. The central region exhibits a concentrated, brighter luminosity, possibly indicating a dense stellar population or active galactic nucleus. Moving outwards from the center, the luminosity gradually decreases, displaying a diffuse halo. The color gradient shifts from a yellow-orange core to a slightly bluer periphery. There is no apparent spiral arm structure or significant dust lane obscuration visible in this imagery. The overall impression is that of a relatively evolved galaxy, likely with a low ongoing star formation rate. There appears to be no major morphological disturbance indicative of recent merger activity, although minor asymmetry might suggest past interaction.
