The galaxy presents a generally smooth morphology, appearing elliptical or lenticular in shape. A central bulge is clearly visible, exhibiting a concentrated luminosity with a yellowish-orange hue, suggesting a population of older stars. Diffuse, bluer light extends outwards from the bulge, implying the presence of a more distributed stellar population. There is a slight asymmetry in the overall light distribution. Evidence of a faint, extended halo may be present, with a subtle transition from the main body of the galaxy to the background sky. The galaxy exhibits no readily discernible spiral arm structure or prominent dust lanes. The color gradients suggest a radial variation in stellar populations, with a potentially ongoing, but low-level, star formation activity in the outer regions. Overall, the galaxy appears to be a relatively evolved system.
