The galaxy presents an elliptical morphology, elongated with a cigar-like shape. Its light profile appears smooth and featureless, suggesting a lack of significant spiral arm structure or prominent dust lanes. The color gradient indicates a concentration of older stellar populations within the galaxy's core, exhibiting a yellowish hue. The outer regions appear slightly less luminous. There is no evidence of recent major merging activity or significant tidal disturbances. The galaxy exhibits intermediate redshift. Based on the observed features, the galaxy is likely a relatively massive system with a suppressed star formation rate.
