The galaxy presents as a relatively smooth, centrally concentrated object, exhibiting a morphology consistent with an elliptical or lenticular galaxy. There is no obvious spiral arm structure or significant dust lane obscuration visible in this image. The central bulge appears bright and somewhat diffuse, with the light gradually diminishing towards the outer regions. The overall shape is approximately elliptical, showing a slight degree of elongation. There is no strong evidence of ongoing merging activity or major tidal disturbances in the immediate vicinity of the galaxy based on this image. The color gradient suggests a population of older stars dominating the light output, although a hint of bluer hues in the outer regions may indicate some limited, ongoing star formation.
