The galaxy presents as a smooth, elliptical morphology with a high degree of central concentration. Its light profile is dominated by a bright, yellowish core, indicative of an older stellar population. The overall shape is somewhat elongated, though it deviates only slightly from a circular form. There is little evidence of spiral arms or distinct features associated with ongoing star formation, though faint blueish tinges are present in the outer regions. The galaxy does not appear to be actively merging or undergoing significant tidal interactions with neighboring galaxies, although there are hints of minor disturbances. The light distribution suggests a relatively evolved system with a likely low specific star formation rate.
