The galaxy presents as a moderately luminous elliptical galaxy, exhibiting a smooth, largely featureless morphology. It appears elongated in shape, with an aspect ratio suggesting it is viewed at a significant angle. The light profile indicates a centrally concentrated luminosity distribution, typical of elliptical galaxies. The color index implies a relatively older stellar population, with a yellow-orange hue indicative of evolved stars, and relatively low levels of ongoing star formation. No obvious signs of spiral arms, dust lanes, or tidal disturbances are apparent. There are no visible features suggesting a recent merger event, and the galaxy appears to be relatively isolated in its environment.
