The galaxy appears to be an elliptical galaxy, exhibiting a smooth, relatively featureless morphology. Its shape is elongated, leaning more towards a cigar-like form rather than perfectly round. The central region is notably brighter and exhibits a reddish-orange hue, possibly indicative of an older stellar population and relatively low levels of ongoing star formation. Moving outwards from the core, the galaxy gradually fades, with subtle bluish tinges appearing in the outer regions. This could suggest the presence of younger, hotter stars in the galactic outskirts, although this is not a prominent feature. The overall impression is that of a mature, quiescent galaxy with minimal signs of significant interaction or disruption. There's no visible evidence of spiral arms, bars, or prominent dust lanes within the observed image.
