The galaxy appears as a somewhat elongated, centrally concentrated object. The color profile suggests a population of older stars, indicated by the redder hues towards the center, and regions of active star formation, indicated by bluer patches throughout, particularly on the outskirts. The galaxy exhibits a generally smooth appearance with some evidence of possible gravitational interaction or tidal disturbance, indicated by a slight asymmetry in its shape and a faint extension on one side. The light distribution is not perfectly uniform, showing some clumpy structures. The overall structure suggests a spiral or lenticular morphology, but with some irregularity indicating it is likely undergoing some type of merger or accretion event.
