The galaxy appears as a centrally concentrated, smooth object with a generally elliptical morphology. The core region exhibits a bright, compact profile that fades gradually into the outer regions. The overall color profile is predominantly yellow, with a slight shift towards red in the fainter, outer regions, suggestive of an older stellar population dominating the galaxy's composition. No distinct spiral arms or significant dust lanes are discernible. There is a very minor visual disturbance, possibly an indication of minor tidal interactions or past merger events. The absence of prominent blue regions suggests a relatively low ongoing star formation rate within the observed timeframe.
