The galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated luminosity profile. Its shape is elongated, deviating noticeably from circularity, with a cigar-shaped appearance. There is a marked absence of spiral arms or distinct disk features. The color is predominantly yellow to orange, suggestive of an older stellar population with a relatively low rate of ongoing star formation. No significant dust lanes or prominent star-forming regions are apparent. The galaxy does not appear to be undergoing any major mergers or tidal disturbances, although subtle asymmetries cannot be entirely ruled out. The overall morphology suggests a galaxy that has largely exhausted its gas reservoir and is populated by aging stars.
