The galaxy presents as a relatively smooth, centrally concentrated object with a distinct yellowish hue. The central region appears significantly brighter and more concentrated than the outer regions. The overall shape is largely round, showing minimal deviations from a circular morphology. There is little evidence of distinct spiral arms or a prominent disk structure. Some faint, irregular extensions of light, potentially tidal features, are barely visible. There are some regions of redder and bluer light, indicating a range of stellar populations, though these features are subtle, overall suggesting relatively low levels of star formation.
