The galaxy presents a primarily smooth and concentrated morphology, with an apparent lack of significant spiral arm structures or prominent dust lanes. The color profile indicates a central concentration of older stellar populations, exhibiting a yellowish-red hue. There is little evidence of active star formation regions within the central region of the galaxy, with faint blue areas sparsely surrounding the galactic bulge. The galaxy's shape appears to be moderately rounded, with no major disturbances or indications of ongoing merging events detectable in the image. Overall, the galaxy is consistent with an elliptical or lenticular type, dominated by evolved stars and a relatively quiescent star formation rate.
