The galaxy presents a largely smooth and rounded morphology. The central region exhibits a concentrated luminosity gradient, appearing bright and somewhat reddish in color, suggesting a population of older stars or dust obscuration. Moving outward from the core, the galaxy gradually fades into a less defined halo of bluish light. This diffuse halo could indicate the presence of a younger stellar population or ongoing star formation, though the smoothness suggests that the rate of star formation may be relatively low. There is no obvious spiral structure or bar visible. There is no distinct evidence of recent major mergers or tidal disturbances in the immediate vicinity of the galaxy. Overall, the galaxy appears to be a relatively quiescent system, likely an elliptical or lenticular galaxy at intermediate redshift.
