The galaxy presents a disturbed morphology, possibly indicative of an ongoing or recent merger event. The system appears to consist of two distinct luminous components. The primary component exhibits a yellowish hue, suggesting a population of older stars, potentially within a spheroidal or elliptical structure. The secondary component is bluer in color, hinting at ongoing star formation. A faint bridge of material seems to connect these two components, further supporting the interaction hypothesis. Overall, the galaxy is of intermediate size and exhibits irregular features, making it difficult to classify using a standard Hubble sequence. Further spectroscopic and photometric analyses are needed to fully characterize the properties of each component and confirm the nature of the interaction.
