The galaxy presents as a relatively smooth, elongated structure with a discernible central bulge. There are no prominent spiral arms visible. The galaxy exhibits a gradual decrease in surface brightness from the core outwards. Color gradients are present; the central region appears whiter, possibly indicating a population of older stars. The outer regions show a bluer hue suggesting the presence of younger stellar populations or ongoing star formation, though no distinct star-forming regions are observed. The shape is somewhat elliptical, with a hint of a disk-like component viewed at an angle. There appears to be minor tidal disturbance. The overall morphology suggests a galaxy in transition, possibly evolving from a spiral towards a more elliptical form.
