The galaxy presents as a elongated spheroid with a concentrated central bulge. The light distribution is relatively smooth, with no obvious spiral arm structure. A color gradient is discernable, shifting from a yellowish hue in the central region to a slightly bluer tint towards the outer edges. This potentially indicates a difference in stellar populations, with older stars concentrated in the core and younger stars more prevalent in the surrounding disk. The galaxy is seemingly undisturbed, displaying no signs of major mergers or tidal interactions. The smooth morphology and color profile suggest a lack of significant recent star formation.
