The galaxy presents as a relatively smooth, disk-shaped structure, exhibiting a dominant central bulge. The disk is viewed nearly edge-on. Evident dust lanes are present, obscuring some of the starlight within the disk and contributing to its reddish hue. Star formation appears to be relatively low. The central bulge appears smooth and concentrated. There is slight evidence of tidal distortion, possibly indicating past or ongoing minor interactions with neighboring galaxies. The galaxy’s overall shape is fairly regular, though there is a slight asymmetry in the distribution of light within the disk. The galaxy is generally isolated.
