Observed galaxy presents a relatively smooth morphology, suggestive of an elliptical or lenticular type. The central region exhibits a concentrated luminosity, characterized by a yellowish hue, possibly indicating an older stellar population and reduced star formation activity. The galaxy appears largely spheroidal with a high degree of roundness, showing minimal evidence of a prominent disk structure or spiral arms. There are no readily apparent signs of significant tidal disturbances or ongoing major mergers. A slight asymmetry might suggest a minor interaction or internal process. The galaxy is relatively compact with no extended halo or diffuse emission visible in this image.
