The galaxy presents as a relatively smooth, centrally concentrated object. The light profile appears to decline gradually from a bright core, suggesting a spheroidal morphology.  The shape approximates roundness, with a subtle deviation towards an elliptical form. There is little evidence of distinct spiral arms or pronounced disk features. Overall, the galaxy exhibits a blueish hue, potentially indicating moderate to low levels of ongoing star formation. There is a lack of significant tidal features or morphological distortions, suggesting it is likely not undergoing a major merger event.
