The galaxy presents as an elliptical system, exhibiting a generally smooth morphology with a centrally concentrated light distribution. Its overall shape is observed to be more "in-between" than distinctly round or cigar-shaped. There is a hint of disturbance or possible minor merging activity in the galaxy's outer regions. The light is observed to be brighter in the redder bands, particularly in the core, with a gradual fading towards the outer edges. This color gradient indicates an aging stellar population. The apparent absence of prominent spiral arms or distinct dust lanes suggests that the galaxy is nearing the end of its star forming life. The galaxy appears to be in a relatively isolated environment with minimal interaction.
