The galaxy appears as a relatively compact and smooth elliptical or lenticular system, with a high degree of central concentration. The light distribution is largely uniform across the main body, suggesting an older stellar population. The color gradient indicates a bluer center, gradually reddening towards the edges. There is some evidence of minor tidal features or disturbances in the morphology, possibly hinting at past or ongoing interaction, but this does not appear to be a major merger event. The overall appearance is consistent with a quiescent galaxy with low levels of recent star formation, and relatively little gas content.
