This galaxy presents as an elongated, cigar-shaped structure. There appears to be a primary concentration of light, indicative of a central bulge or core region. A less defined, secondary region of brightness is also visible, suggesting some asymmetry within the galactic structure or potential tidal disturbances. The overall color profile leans towards the redder end of the spectrum, hinting at an older stellar population and/or significant dust obscuration. There is some evidence of star formation, specifically in the bluer hues, although relatively subdued, within the galaxy. No significant signs of a major ongoing merger are readily apparent, but minor disturbances or interaction cannot be ruled out. Overall, the galaxy appears to be a somewhat evolved system with hints of past interactions.
