The galaxy appears as a centrally concentrated object with a generally smooth morphology. Its shape is approximately round, exhibiting a slight elongation. Coloration suggests an older stellar population dominating the light output, with a yellowish-red hue. There is no clear evidence of distinct spiral arms or a prominent disk structure. Subtle irregularities may suggest a minor gravitational disturbance or interaction, although a merger event is not definitively apparent from this image alone. The overall impression is that of a relatively massive galaxy with a low star formation rate.
