The galaxy appears as a single, luminous object, showing a generally elliptical morphology. The light distribution suggests a centrally concentrated structure, with a smooth, diffused appearance. A very slight elongation is seen, but overall, the galaxy presents a rounded form. There is an apparent lack of distinct spiral arms or prominent dust lanes typically associated with disk galaxies. The color profile shows a tendency toward warmer, redder hues. No evidence of ongoing major mergers or tidal disturbances is immediately obvious. Based on these observations, it is probably an early-type galaxy, specifically an elliptical or lenticular galaxy.
