The galaxy presents a moderately luminous appearance, with a relatively smooth overall structure. It appears to be an elliptical galaxy, exhibiting a somewhat elongated shape rather than a distinct spiral arm structure. The central region of the galaxy displays a concentrated area of higher luminosity, suggestive of a prominent galactic nucleus. There is evidence of some morphological disturbance, as the shape is not perfectly symmetrical; this could possibly be due to tidal interactions. The galaxy shows a bluer color profile in its outer regions compared to the core, indicating ongoing star formation. There are no prominent dust lanes visible, and no clear signs of a recent major merger. The overall light distribution indicates that it's likely a fairly massive galaxy.
