This galaxy appears to be a relatively smooth, centrally concentrated system with a moderate redshift. Its morphology suggests a mostly featureless spheroid, exhibiting a flattened but not strongly disk-like structure. The overall color profile tends toward the redder end of the spectrum, with a bright yellow core possibly indicative of an older stellar population or dust obscuration. There is some asymmetry visible in the form of a slightly extended arm on the right side, indicating that it may have had a minor merger in the past. The extent of the galaxy is relatively small, with a high likelihood of being a spheroid structure. There may be a small amount of star formation within the galaxy, but it is likely not significant.
