The galaxy presents a generally smooth morphology. It appears largely elliptical, exhibiting a radial concentration of light towards the center. The core is a yellowish-orange hue, possibly indicative of an older stellar population, with the concentration of light suggesting a high stellar density in this region. Moving outward from the core, the color shifts to a slightly greenish tint, with the overall luminosity decreasing with radial distance. A very slight asymmetry can be noted in the shape, with the galaxy being somewhat elongated. There does not seem to be significant evidence of spiral arm structures, strong dust lanes, or tidal tails. No signs of active galactic nuclei are immediately apparent. The object shows some signs of possible minor gravitational interaction.