The galaxy presents a largely smooth morphology, with approximately spherical symmetry. A concentrated central bulge is visible, appearing a yellow-white hue. The surrounding disk exhibits a bluish tint, indicating the presence of younger stellar populations. Some irregularities are noted. It shows little evidence of active merging or significant tidal disturbances and is likely in a relatively settled state. Considering an estimated radius of roughly 4.4 kpc, this galaxy would be characterized as intermediate in size. Overall, this appears to be an intermediate-sized galaxy showing signs of active star formation, with a dominant smooth morphology.
