The galaxy presents as a largely featureless elliptical or lenticular type, exhibiting a smooth luminosity profile with a concentrated central bulge. Its color is predominantly yellowish-orange, suggesting a population dominated by older stars. The galaxy appears somewhat elongated, deviating slightly from a perfectly circular morphology. There might be a faint, diffuse halo surrounding the brighter central region. No distinct spiral arms or dust lanes are discernible. Given the smooth appearance and color, this galaxy likely has a relatively low star formation rate. There appears to be minor distortion within the galaxy, with some irregularities in the light distribution that could indicate a previous or ongoing minor interaction.
