This galaxy presents a generally smooth and concentrated appearance. Its overall shape is more elongated than circular but not extremely so, exhibiting an intermediate axial ratio. The color profile reveals a central region that is slightly more yellow, suggesting an older stellar population. This contrasts with the outer regions which appear bluer, indicative of recent star formation. There are no distinct spiral arms or a prominent disk structure that can be visually identified. The galaxy does not appear to be undergoing any major merging activity, although there may be minor irregularities.
