This galaxy presents a disk-like morphology, viewed at an inclined angle relative to our line of sight. The central bulge appears prominent, exhibiting a concentrated brightness indicative of a high stellar density, possibly an elliptical or lenticular structure. The disk exhibits spiral arm structures, though they are not sharply defined. The spiral arms exhibit a patchy distribution of light, potentially indicating regions of active star formation. The galaxy appears to be relatively isolated, with no obvious signs of ongoing major mergers or strong tidal interactions with neighboring galaxies. Overall, it has the appearance of a relatively undisturbed galaxy, with a possible bar structure in the center.
