This galaxy presents as a relatively smooth and diffuse structure, displaying a central bulge that dominates its overall appearance. The light distribution appears to be elongated, suggesting an elliptical morphology, albeit one that is not perfectly spherical. There is minimal evidence of distinct spiral arm structures or prominent dust lanes, indicating a lack of significant ongoing star formation. The galaxy's color is generally uniform, with subtle variations in intensity across its surface. There may be signs of a minor gravitational disturbance, but the galaxy is not undergoing any major merging events.
