The galaxy presents as a centrally concentrated object with a generally smooth morphology. It exhibits a distinct yellowish-orange hue, suggesting a stellar population dominated by older, evolved stars and a relatively low rate of ongoing star formation. The light distribution appears largely spheroidal, indicating a possible elliptical galaxy or a lenticular galaxy seen face-on. There is little evidence of prominent spiral arms or dust lanes. No obvious signs of recent merger activity or major tidal disturbances can be observed. The galaxy shows an overall compact appearance with a moderately bright core, gradually fading toward its periphery.
