The galaxy presents as a somewhat elliptical structure with a smooth, concentrated central bulge. The color profile appears to be centrally concentrated with yellower hues, suggesting an older stellar population dominates the core. The outer regions are less defined, with hints of bluer colors, implying the presence of some younger stars or ongoing star formation. There may be a very faint disk component present, but is not well defined. No strong spiral arm structures or other distinct features are visible. The galaxy does not appear to be undergoing any major mergers or exhibiting significant tidal disturbances.
