The galaxy appears as a centrally concentrated object, exhibiting a generally elliptical morphology. The light distribution is relatively smooth, lacking prominent spiral arm structures or significant dust lanes. The galaxy's color suggests a moderate stellar population age, leaning towards a slightly redder hue, implying the presence of older stars and potentially ongoing, but not vigorous, star formation. There is a subtle hint of a disk-like structure within the overall elliptical shape. No major disturbances or signs of ongoing mergers are immediately apparent. Based on the overall appearance, this galaxy is likely an intermediate mass system, with a fairly high rate of star formation.
