The galaxy presents as a moderately small, diffuse object with an overall blue hue. The light distribution appears relatively smooth, suggesting a lack of prominent spiral arms or a well-defined bulge. There are no distinct knots of star formation visible, indicating a relatively low current star formation rate. The overall morphology suggests a potentially late-type or irregular galaxy, though a heavily obscured spiral cannot be ruled out. Some level of disturbance is indicated by the slight asymmetry in the galaxy's light distribution, and this could be evidence of minor interaction with another galaxy, or perhaps a recent merger event. The outer regions appear less defined, hinting at an extended halo of stars or gas. The galaxy's relatively low mass makes it appear likely that the galaxy is dominated by dark matter. 
