The galaxy presents a generally smooth appearance, suggesting a likely classification as an elliptical or lenticular type. Its overall shape approximates a slightly elongated spheroid, with the degree of ellipticity being moderate, tending towards a somewhat round shape. A central bulge region is noticeable, exhibiting a brighter, more concentrated luminosity compared to the outer regions. There is some suggestion of a faint, diffuse disk, but this is not strongly defined. The galaxy displays a color gradient, with the central regions appearing redder, potentially indicating an older stellar population, while the outer regions show hints of bluer hues, possibly suggesting the presence of some younger stars or ongoing star formation, albeit at a modest rate. There is no evidence of any major morphological disturbances, such as tidal tails or obvious signs of a recent merger, although minor irregularities or asymmetries cannot be entirely ruled out given the image resolution.
