The galaxy appears as a centrally concentrated object with a relatively smooth morphology. It exhibits a generally elliptical shape, appearing mostly round with a slight deviation from perfect circularity. There are no strong indications of prominent spiral arm structures or a well-defined disk. The galaxy's light is dominated by a redder hue in its central region, possibly indicating an older stellar population. There's a gradual fading of luminosity from the core to the outer edges, forming a fairly defined boundary. No significant signs of ongoing major mergers or tidal disturbances are readily apparent, though there might be a very faint asymmetry suggesting a minor interaction.
