The galaxy presents a generally smooth appearance, with hints of some internal structures. The light distribution suggests a central bulge, surrounded by a fainter, more extended component that could be a disk. The galaxy appears to be somewhat elongated in shape, but not extremely so. The dominant color is reddish, suggesting an older stellar population and potentially less active star formation. There are potential signs of minor disturbances or asymmetries in the galaxy's morphology, hinting at possible past interactions with other galaxies. However, the galaxy does not appear to be undergoing a major merger. The galaxy has a substantial mass.