The galaxy appears as a somewhat elongated, lenticular-shaped object with a relatively smooth light distribution. The central region exhibits a more concentrated, yellowish-orange hue, suggesting an older stellar population. Extending outward from the core is a less defined, bluer envelope of light, perhaps indicative of more recent star formation activity. The overall color gradient transitions from warmer tones at the center to cooler tones in the outer regions, but the color differences are not drastic. There is no obvious spiral structure or defined dust lanes visible. The object appears to be quite compact and regular in its morphology, lacking any signs of major disturbances or tidal features. The high degree of ellipticity suggests that it may be an edge-on disk galaxy.
