The galaxy presents as an elliptical morphology, with a smooth light distribution lacking distinct spiral arms or a prominent central bulge. It appears elongated, with an axial ratio indicating it is not perfectly spherical. The color profile suggests an older stellar population, as evidenced by the reddish-gold hue concentrated towards the center. The outer regions exhibit a slightly bluer tint, possibly indicating the presence of some younger stars, although this feature is not prominent. There are no readily apparent signs of ongoing major merging activity or significant tidal disturbances. The galaxy appears to be relatively isolated, with no nearby galaxies showing signs of strong interaction.
