The galaxy appears to be a relatively small, elongated structure. Its color profile suggests a bias towards redder hues, which could imply an older stellar population with fewer active regions of star formation. The galaxy's morphology does not exhibit clear spiral arms or a well-defined disk, and appears somewhat amorphous. There is evidence of minor disturbances and/or possible interaction with another galaxy. It could potentially be undergoing a merger. The core of the galaxy shows a slightly brighter concentration of light.