The galaxy exhibits an elliptical morphology, appearing largely smooth with a high degree of central concentration. The light distribution suggests a centrally dominant bulge component. The galaxy's color profile indicates the presence of an older stellar population, with an overall yellowish-red hue. There are some indications of bluer light near the center, possibly hinting at ongoing or recent star formation. The galaxy shows no strong evidence of spiral arm structure or significant dust lanes. The overall impression is that of a relatively evolved system, potentially in the process of quiescence. There is no prominent tidal stream or indication of recent major merger event. 
