The galaxy appears as a slightly elongated structure with a bright, concentrated central bulge. Surrounding the bulge, there is a fainter disk component that extends outwards, more so in one direction than the other. The color distribution suggests a relatively redder bulge, indicative of an older stellar population. The disk shows some evidence of bluer regions, possibly indicating areas of more recent star formation activity, or perhaps a dusty disc. The overall morphology suggests the galaxy is likely a spiral or lenticular galaxy, though without higher resolution imaging, definitive classification is difficult. There may be some minor distortions present which could suggest a history of interaction or ongoing minor merger activity.
