The galaxy exhibits an elliptical morphology, appearing largely smooth with a slight elongation. There is a noticeable concentration of light towards the galaxy's center, suggesting a prominent bulge. The color profile indicates an older stellar population, particularly towards the center, exhibiting redder hues. Fainter blueish regions are visible, particularly along the periphery, possibly indicative of some ongoing, albeit minimal, star formation. There does not appear to be any strong evidence of spiral arms or a well-defined disk structure. Minor irregularities in the light distribution could point to past or ongoing minor interactions, but the overall structure remains relatively undisturbed. The lack of significant dust lanes further supports the assessment of a relatively quiescent system.
