The galaxy appears as a somewhat smooth, centrally concentrated object with a slight elongation. Its color profile suggests a dominant older stellar population, with a yellowish-orange hue. There is a subtle hint of bluer light in the central region, potentially indicating ongoing or recent star formation activity, albeit at a relatively low rate. A slight asymmetry in the outer regions of the galaxy could indicate a minor gravitational interaction or past merger event, although no major disturbances are readily apparent. The object's overall form is relatively round. The galaxy's relatively compact size suggests a low to intermediate mass range.
