The galaxy presents as a lenticular or early-type spiral, with a bright, relatively featureless central bulge dominating its overall appearance. The bulge exhibits a smooth light distribution, suggesting an older stellar population with minimal ongoing star formation. Faint extensions emanate from the central region along the major axis, potentially indicative of a nascent or truncated disk structure. These outer regions appear less structured than typical spiral arms and contribute to the galaxy's elliptical shape. There is no clear evidence of significant dust lanes or prominent spiral arm features within the visible spectrum of this image. The galaxy appears moderately inclined relative to our line of sight. Overall, the galaxy exhibits a redder hue, consistent with a relatively evolved system.
