This galaxy presents as a somewhat elliptical, relatively smooth object. There is a prominent, concentrated central bulge displaying a yellowish hue. This could indicate an older stellar population within the core. Surrounding the bulge is a fainter, more diffuse disk or halo component, with a bluer tint suggesting the presence of younger, hotter stars, and possible ongoing star formation. There appears to be a very slight disturbance in the halo region, perhaps indicating a minor interaction. The galaxy lacks any well-defined spiral arm structure or dust lanes that would be indicative of a disk galaxy undergoing significant star formation.
