The galaxy presents as a relatively compact object. It exhibits a generally smooth morphology, with a slight elongation but lacks any obvious spiral arm structures or a prominent central bulge. The galaxy's color profile leans towards the blue end of the spectrum, suggesting the presence of a younger stellar population and ongoing star formation, though perhaps at a moderate rate. There are no apparent signs of major mergers or significant tidal disturbances in its immediate vicinity. The galaxy appears to be fairly isolated.
