The galaxy presents as an elliptical morphology, appearing relatively smooth in texture. A concentrated central bulge dominates the structure, displaying a yellowish hue, suggestive of an older stellar population. Extending outward from the central bulge, there is a fainter, more diffuse disk component. Faint blue tinges are visible in this disk, possibly indicating the presence of some younger, hotter stars and potential ongoing, albeit mild, star formation. There is no obvious presence of spiral arms or any other distinct morphological features such as bars or rings. Overall, the galaxy appears to be relatively undisturbed, without any evidence of ongoing major mergers or tidal interactions. The galaxy's apparent shape indicates that it is not viewed face-on, and instead is at an oblique viewing angle relative to our line of sight.
