The galaxy presents as a single, relatively smooth object with a moderately elongated shape. Its morphology appears to be intermediate between a perfectly round and a cigar-shaped form. The galaxy exhibits a central concentration of light, with a diffuse, extended halo or envelope surrounding the core. There may be some slight irregularities in its structure, with the suggestion of minor disturbances. Overall, it seems to be a relatively isolated galaxy with no obvious signs of major interactions or mergers. The galaxy displays variations in color, with bluer regions possibly indicating areas of younger star formation. The estimated size of the galaxy is approximately 5 kiloparsecs. The rate of star formation is relatively low.