This galaxy exhibits a predominantly smooth morphology, with a highly elongated, cigar-like shape. There is minimal evidence of spiral arm structures or distinct star-forming regions within the observable light. The light distribution suggests a concentrated central bulge which fades gradually into the outer regions. It shows a yellow-red hue, suggesting a population of older stars and lower ongoing star formation. There are no signs of any major merger events, however, a minor disturbance cannot be ruled out.
