The galaxy appears to be an elliptical or lenticular type, exhibiting a relatively smooth and featureless morphology. It is characterized by a centrally concentrated bulge of light that is slightly elliptical, exhibiting an axis ratio that is approximately 0.8. The galaxy shows a smooth light distribution that diminishes gradually from the core, with no evidence of spiral arms or prominent dust lanes. There is a very faint halo surrounding it. There is a slight color gradient, with the central regions appearing slightly yellow-white, suggesting an older stellar population. The galaxy’s overall appearance is indicative of a system where star formation has largely ceased, and the dominant population is composed of older, redder stars. It shows no evidence of any major tidal disturbances or ongoing mergers.
