The galaxy presents as a relatively smooth, centrally concentrated object with a largely elliptical morphology. There is a distinct lack of prominent spiral arm structures. The light profile appears to gradually decrease from the bright central bulge outwards to the faint outer regions. The galaxy has a noticeable yellowish-white hue, suggestive of an older stellar population. There is no strong evidence of ongoing major star formation as indicated by the lack of blue regions. The galaxy shows a fairly regular structure, with no obvious tidal tails or distortions indicative of recent major merger events, although there is the slightest hint of minor asymmetry. Overall, it appears to be a mature galaxy in a relatively quiescent state.
