The galaxy presents an elliptical morphology, appearing largely smooth and centrally concentrated. The core exhibits high luminosity, transitioning to a fainter, more diffuse halo. There is evidence of possible minor disturbances, hinted by subtle asymmetries in the halo structure. The overall color profile skews toward the blue end of the spectrum, potentially indicating recent or ongoing star formation activity within the galaxy, although the smoothness suggests a lack of spiral arm structure. There is a distinct, yet subtle edge to the galaxy, perhaps indicative of a tidal interaction. Further spectroscopic analysis is needed to determine the redshift, stellar population characteristics, and confirm potential merging activity.
