The galaxy presents as a roughly elliptical structure, exhibiting a relatively smooth, though not perfectly uniform, light distribution across its body. There is a slight elongation, suggesting it may not be perfectly spherical. The galaxy appears to have a redder hue, indicating an older stellar population, and potentially significant dust content. No distinct spiral arms or prominent features are readily visible. The overall morphology suggests a lack of ongoing major star formation. Subtle color variations within the galaxy could indicate regions of differing stellar populations or dust concentrations. There is no apparent central bulge dominating the galaxy's structure. The galaxy appears relatively isolated, showing no obvious signs of major interaction or merging with another galaxy. There may be a suggestion of minor tidal features, however this can be difficult to confirm due to the image resolution.
