The galaxy presents a generally smooth morphology, appearing largely featureless in this image. Its shape is elliptical, with a noticeable elongation. The light distribution suggests a centrally concentrated luminosity profile, fading gradually outwards from a bright, dense core. The color is generally redder throughout, especially towards the center. There is no obvious spiral structure or prominent dust lanes. The galaxy exhibits no clear signs of major interactions or mergers, though minor disturbances cannot be ruled out at this resolution. The observed red color and smooth morphology are indicative of a galaxy populated by an older stellar population with relatively low on-going star formation.
