The galaxy presents a somewhat amorphous structure, potentially indicative of an ongoing or recent merger event. There is a primary, brighter core region with a concentrated luminosity. A secondary, distinct luminous region is observed at a slight offset, possibly a remnant core of a merging galaxy or an area of intense star formation activity. The primary core exhibits a bluer hue, suggestive of a younger stellar population and/or ongoing star formation. Fainter, diffuse material surrounds both luminous regions, exhibiting a more redshifted color. Overall, the light distribution appears disturbed, supporting the hypothesis of gravitational interaction and indicating that the galaxy is undergoing a period of dynamic evolution.
