The galaxy presents as a relatively smooth and centrally concentrated object, with a noticeable decrease in luminosity from the core outwards. The light distribution appears fairly even, with a slight elongation but no distinct spiral arm structures visible. Color analysis suggests a population of older stars, primarily in the redder portion of the spectrum, with a lower contribution from bluer, younger stars. There's no clear evidence of active star formation regions within the observed bands. The lack of significant tidal tails or obvious distortions indicates no recent major merger activity. However, there may be some minor disturbances within the galactic structure. The galaxy can likely be classified somewhere between an elliptical and a lenticular galaxy, based on the smooth light profile and lack of visible spiral structures.
