The galaxy appears to be a relatively smooth, round-shaped object. It exhibits a bright, concentrated central bulge. The light profile suggests a gradual decline in intensity from the core outwards, consistent with an elliptical or S0 galaxy morphology.  The colors are predominantly red and yellow, which suggests an older stellar population with lower levels of ongoing star formation, although there is a hint of some bluer light on the edges. There is no obvious evidence of spiral arms or significant dust lanes. The object does not appear to be undergoing any major merger activity or tidal disruption.
