The galaxy presents a somewhat irregular, elliptical morphology. A central bulge region exhibits a yellowish-white hue, indicative of an older stellar population. Surrounding this core, a fainter, bluer halo extends outwards. This blue color suggests the presence of younger, hotter stars, possibly in regions of ongoing star formation. There's a slight asymmetry to the galaxy's overall shape, possibly hinting at tidal interactions or recent minor merger event. A slight disk like feature may be present but disrupted. The galaxy does not have a clear spiral arm structure. Overall, the galaxy shows characteristics of being in transition with elements of both elliptical and spiral galaxies.
