The galaxy presents as an elliptical type, exhibiting a smooth, concentrated light profile. Its overall shape appears largely spheroidal with a slight elongation, suggesting a possible transition between E0 and E3 morphological classifications. The core of the galaxy displays a yellowish hue, indicative of an older stellar population, potentially dominated by red giant stars. Moving outward from the core, the galactic halo exhibits a bluer tinge, suggesting the presence of younger, hotter stars, possibly tracing regions of more recent star formation activity. There's no clear indication of significant spiral arm structures or dust lanes from this view. The galaxy does not appear to be undergoing a major merger, though some minor tidal disturbances can not be ruled out. Overall, this galaxy appears as a moderately luminous elliptical system, possibly still undergoing some limited star formation.
