The galaxy presents a generally smooth and rounded morphology. Its color profile suggests an older stellar population, dominated by yellow and red hues. There is little evidence of spiral arm structure or significant dust lanes. The galaxy appears to be relatively isolated, with no obvious signs of tidal disruption or interaction with nearby galaxies. The light is centrally concentrated, indicative of a well-defined galactic nucleus. A faint, diffuse halo extends beyond the bright core. Based on its morphology and color, this galaxy likely represents an elliptical or lenticular system undergoing a relatively low rate of star formation.