The galaxy appears to be an elliptical or lenticular type, exhibiting a generally smooth morphology. There is no clear evidence of spiral arms or a prominent disk structure. The galaxy's shape is somewhat elongated, though tending more toward being round. Its central region presents a brighter, more concentrated luminosity, suggesting a significant stellar population density or a possible active galactic nucleus. There's subtle color variation across the galaxy, with the central region showing a slightly yellowish hue, potentially indicating an older stellar population, while the outer regions exhibit a fainter, bluish tinge suggestive of younger stars, or the effects of redshift. There are no obvious signs of major merger events or significant tidal disturbances. A very slight asymmetry is present, but is not considered significant given the smooth overall distribution of light.
