The galaxy appears to be a relatively face-on spiral galaxy with a prominent bulge and a moderately inclined disk. The central bulge is a concentrated region of luminosity, appearing smooth and yellowish-white, suggesting an older stellar population. The disk appears to be slightly inclined, with a higher concentration of light towards the center. The spiral arms appear somewhat faint and patchy, displaying a bluer color indicative of ongoing star formation, though the rate seems relatively moderate based on the absence of highly luminous HII regions. The overall shape of the galaxy is elliptical. There are no obvious signs of a major merger or significant tidal disturbances. The galaxy has an estimated diameter of around 3 kiloparsecs.
