The galaxy presents as a spheroid with a significantly elongated morphology, approximated as a prolate spheroid when considering its three-dimensional structure. The central region exhibits a concentrated luminosity profile, suggesting a high density of stars in the galactic nucleus. A color gradient is observed across the galaxy, with the central bulge displaying a distinctly redder hue, potentially indicative of an older stellar population and a higher concentration of dust. Fainter, bluer regions appear distributed throughout the outer areas of the galaxy, possibly indicating regions of recent or ongoing star formation, although these features are not sharply defined. No spiral arm structure or prominent dust lanes are discernible in the image. Faint tidal features cannot be ruled out. Overall, the galaxy appears largely undisturbed.
