The galaxy appears to be a lenticular or early-type spiral, exhibiting a smooth, elongated morphology reminiscent of a flattened spheroid. It has a central bulge that is dominated by older stars, which appears yellowish-orange in color, suggestive of an aging stellar population with low current star formation. The disk is faint, with a hint of blue color at the edges, and a faint dust lane that contributes to the observed redness of the bulge. There appear to be no obvious spiral arms or signs of active star formation regions. The galaxy shows no significant signs of tidal disturbances or interactions with other galaxies.
