The galaxy presents a roughly elliptical morphology, appearing largely smooth with a concentrated central bulge. The core region exhibits a bright, relatively uniform luminosity across the observed optical wavelengths, suggesting a high density of stars. A faint, diffuse halo extends outwards from the core, displaying a subtle elongation along a preferential axis. The color gradient is slight, with a tendency towards bluer tones in the outer regions, possibly indicative of ongoing star formation. Subtle irregularities in the halo's luminosity suggest potential minor disturbances or interactions. There is no clear evidence of prominent spiral arms or a well-defined disk structure. Overall, the galaxy seems to be an early-type system, likely an elliptical or lenticular galaxy, showing minor signs of recent or ongoing interaction.
