The galaxy presents a generally smooth morphology, with a notable lack of distinct spiral arms or prominent dust lanes. The light distribution appears centrally concentrated, with a gradual decrease in intensity towards the outer regions. The shape is elongated, exhibiting an elliptical form rather than a circular one. There is a hint of color variation across the galaxy, with a slightly redder hue towards the central region and a subtle bluer tint in the outer areas. This could indicate a gradient in stellar populations or dust content. There's no apparent signs of major mergers or significant tidal disturbances. The galaxy exhibits a fairly quiescent state, indicative of a relatively low star formation rate.
