The galaxy appears to be of intermediate size, possessing a central bulge that is elongated. The bulge exhibits a yellowish hue, suggestive of an older stellar population. Surrounding the bulge is a fainter, bluer disk component, indicating the presence of younger stars and possibly ongoing star formation. The disk appears slightly disturbed, showing some asymmetry. There may be subtle signs of tidal features, hinting at a possible past interaction or merger event, but the disturbances may also be explained by internal factors. The galaxy is neither perfectly elliptical nor a well-defined spiral, presenting a morphology somewhere in between.
