The galaxy presents as an elliptical morphology, exhibiting a largely smooth, concentrated light profile. The central region is dominated by a bright, yellowish-white core, possibly indicative of an older stellar population. There is a subtle, diffuse extension of light surrounding the core, fading into the background. The shape appears to be somewhat elongated but still maintains a generally rounded overall form. No prominent spiral arm structures or significant dust lanes are visible. There are no obvious signs of recent major merger activity, such as tidal tails or shell structures. There appears to be a hint of blue in the outer regions, suggesting the presence of some younger stars.
