The galaxy exhibits an overall smooth morphology with a relatively round shape. The light distribution appears concentrated towards the center, suggesting the presence of a bulge. There is no apparent spiral arm structure or bar visible. The color of the galaxy is fairly uniform, with a slight color gradient towards the center indicating a possible variation in stellar populations or dust content. The galaxy appears relatively isolated, with a possibility of minor disturbance in the morphology suggesting a potential interaction. There is also a faint, elongated object nearby that may be a tidal tail or another galaxy involved in an interaction.