The galaxy presents an elongated, cigar-shaped morphology. Its color profile suggests a dominant population of older stars, appearing generally redder than galaxies with ongoing active star formation. The central region exhibits a brighter, more concentrated luminosity, suggestive of a galactic bulge. Evidence of spiral arm structures or distinct star-forming regions is not readily apparent from the image. The smooth appearance is indicative of a relatively evolved system, potentially an elliptical or lenticular galaxy. Overall, the galaxy exhibits a morphology consistent with a non-disturbed system, showing no signs of major merging events.