This galaxy presents as a relatively smooth, elongated structure. The light distribution suggests it's primarily an elliptical galaxy, though a slight hint of a disk-like structure is present. The galaxy appears to be cigar shaped. The light gradient transitions smoothly from the core outwards, indicating a well-mixed stellar population. There is a redder central region, potentially indicating a concentration of older stars and dust towards the galaxy's core. The color transitions towards bluer hues in the outer regions, possibly indicating more recent star formation activity. Overall, this galaxy appears to be a well-defined elliptical, though with a slight blue tint perhaps indicative of recent star formation. The galaxy does not seem to be undergoing any major merging activity. However, there may be minor disturbances in the outskirts that are not visible in the image, but the galaxy appears to be relatively isolated.
