The galaxy appears to be a relatively smooth, elliptical galaxy. Its light profile exhibits a high degree of central concentration, peaking in a bright, yellowish core. This core gradually fades outward into a more diffuse halo. The galaxy displays an elongated morphology, exhibiting a slight, almost imperceptible disk-like feature. The overall color is indicative of an older stellar population, with a general redder hue particularly dominant in the central bulge, consistent with a population of evolved stars. There is little evidence of significant dust lanes or active star formation regions. The morphology is largely undisturbed, with no clear signs of ongoing or recent mergers, although there may be a minor asymmetry hinting at possible past interaction. The galaxy's form is more akin to being an oblate spheroid rather than an irregular form.
