The galaxy presents as a relatively smooth, elliptical object. It has a notably elongated morphology, appearing cigar-shaped. The central region exhibits a bright, concentrated luminosity, suggesting a dense stellar population and possibly an active galactic nucleus, although further spectroscopic data would be required to confirm this. Moving outward from the core, the luminosity gradually decreases. No distinct spiral arm structures are observed, and there is little evidence of significant dust lanes or prominent star-forming regions. There's a hint of a subtle, extended halo surrounding the main body, but its extent and structure are not clearly defined in this image. Overall, the galaxy seems to be a relatively undisturbed, evolved system with a dominant, spheroidal component. There is no clear evidence of any major ongoing merger activity or tidal interactions.
