The galaxy presents as a relatively smooth, elliptical-like structure, exhibiting a concentrated central bulge. The color profile suggests a dominant population of older stars, contributing to its yellowish hue. There is a small hint of bluer regions near the center, indicating some modest amount of on-going star formation. No obvious spiral arm structure or significant dust lanes are visible. The galaxy appears fairly undisturbed, with no major signs of recent mergers or tidal interactions. Its overall form is generally round and compact.
