The galaxy presents as a single, dominant object with a generally smooth morphology. Its shape approximates a rounded ellipse, exhibiting a subtle elongation. The light distribution is concentrated towards the center, suggesting a prominent galactic bulge. The galaxy appears to be relatively isolated and undisturbed, showing no major signs of interaction with other galaxies. A color gradient exists, with a slightly redder hue towards the central regions, possibly indicating a greater abundance of older stellar populations in the bulge compared to the outer areas of the galaxy. Faint and diffuse light extends outwards from the core, suggesting the presence of a halo or extended disk component.
