The galaxy appears to be a relatively smooth, elliptical system. Its overall color profile is yellowish-red, suggesting a population of older stars and relatively little ongoing star formation. The galaxy's morphology is predominantly spheroidal, exhibiting a high degree of central concentration. There are some faint indications of a possible extended halo or tidal features, but these are not prominent and may require further investigation to confirm. No obvious spiral arm structures or dust lanes are discernible. The galaxy appears relatively isolated, with no immediate signs of major mergers or significant tidal interactions with other galaxies. The galaxy exhibits a high degree of roundness in its overall shape. Based on the magnitude measurements, it's a luminous galaxy.
