The galaxy presents as an object with a relatively smooth morphology. Its overall shape appears somewhat elliptical, with no prominent spiral arm structures or a distinct central bar visible in this image. The color profile suggests a population of older stars, evidenced by the redder hue in comparison to actively star-forming galaxies. There's a potential indication of a minor interaction or disturbance in its form, though the image resolution limits a definitive assessment. The galaxy's light distribution is concentrated toward the center, indicating a bright galactic nucleus. It exhibits considerable luminosity, suggesting a substantial mass.
