The galaxy presents as a centrally concentrated, smooth object with a notable lack of distinct spiral arm structures or significant dust lane features. Its overall shape appears to be elliptical or lenticular, trending towards an elliptical morphology given the dominance of the bulge. There may be a faint flattened disk of relatively low surface brightness. The color profile displays a redder hue compared to typical spiral galaxies, suggesting an older stellar population with diminished recent star formation. Minimal indications of tidal disturbances or ongoing merger events are discernible within the image. The light distribution suggests a fairly even stellar density outward from a bright central core, although subtle variations may be present in higher resolution imaging. The galaxy appears to be in a relatively isolated environment, showing no strong signs of gravitational interactions with nearby galaxies.
