This galaxy appears to be a lenticular or early-type spiral galaxy, exhibiting a smooth, somewhat elliptical morphology. The galaxy is dominated by a central bulge that exhibits a bright, concentrated luminosity profile, likely indicating an older stellar population.

A flattened disk component is visible, though lacking well-defined spiral arms. The disk appears relatively smooth and featureless, suggesting a low rate of current star formation. There is some evidence of a faint blue hue in the disk region, perhaps due to a small population of younger, hotter stars, though the overall color suggests a predominately older stellar population.

The galaxy exhibits an overall intermediate ellipticity, leaning towards a cigar shape, indicating a significant amount of rotational support. There are no obvious signs of recent major mergers or strong tidal interactions.

The galaxy appears to be moderately inclined to our line of sight.
