The galaxy presents as a centrally concentrated system with a relatively smooth appearance. The core exhibits a bright, somewhat diffuse glow, indicating a high density of stars in the central region. Moving outwards from the core, there's a gradual fading in luminosity, forming a more extended halo. Faint hints of blueish light can be seen in this outer region, potentially suggestive of some ongoing star formation. The galaxy appears to be relatively rounded in shape, with no clear signs of spiral arm structures or a prominent disk. There are indications of minor disturbances within the galaxy; these could be tidal effects or minor mergers. Overall, the galaxy's morphology points towards an elliptical or lenticular classification, with some level of recent or continuing star formation.
