The galaxy presents as a relatively smooth, round object. It displays a concentrated central bulge, characterized by a yellowish-orange hue, suggesting a population of older stars. There is very little evidence of spiral arm structure and no indications of any significant ongoing star formation. The overall morphology appears undisturbed, with no apparent signs of tidal features or recent merger events. The galaxy is likely a spheroidal type, potentially an elliptical or an S0 galaxy, dominated by an older stellar population and limited ongoing star formation.
