The galaxy presents as a single, largely homogenous structure. Its overall morphology appears elliptical, with a moderately high degree of central concentration. The light distribution is relatively smooth, exhibiting a gradual decline in intensity from the core outwards, lacking any prominent spiral arms or distinct features characteristic of disk galaxies. The color profile is dominated by yellow-red hues, suggesting a population of older, evolved stars. There is no apparent evidence of significant dust lanes, active star formation regions, or ongoing merger activity. The galaxy appears relatively undisturbed, suggesting a quiescent evolutionary state.
