The observed galaxy presents an overall smooth morphology, suggestive of an elliptical type. The light distribution appears centrally concentrated with a radial falloff in intensity. The galaxy exhibits a slight ellipticity, deviating from a perfect circular shape; it is tending towards being round, though with a more intermediate form. There is a faint suggestion of a minor disturbance present, possibly indicating an interaction or merger event in its past, as there are some slight irregularities in the galaxy's outer regions. No distinct spiral arm features or prominent disk structures are discernible in the image. The galaxy appears to be relatively isolated, with no major merging events drastically distorting its overall form. The image is composed primarily of green wavelengths.