The galaxy presents as a relatively compact object with an overall smooth morphology. It exhibits a slight bluish hue, which may indicate the presence of a young stellar population and ongoing star formation. There is little evidence of distinct spiral arms or a pronounced disk structure. The light distribution suggests a centrally concentrated luminosity profile, with a gradual fading towards the outer regions. The object appears somewhat round, not highly elongated. Subtle asymmetries in the light distribution hint at possible minor disturbances or interactions.
