The galaxy appears as a moderately sized, relatively smooth elliptical or lenticular structure. The light distribution is centrally concentrated, fading gradually outwards from the core, suggesting a lack of significant spiral arms. The overall color is somewhat red, indicative of an older stellar population with suppressed ongoing star formation. There may be subtle deviations from perfect ellipticity, hinting at a possible interaction or minor disturbance, but the primary impression is that of a relatively relaxed system. No prominent dust lanes or bright, blue star-forming regions are apparent. The galaxy presents a smooth and somewhat rounded morphology.
