The galaxy presents an overall hazy, diffuse appearance, with a slightly irregular shape. The central region exhibits a concentrated, yellowish-white hue, suggesting an older stellar population or a significant dust concentration. Surrounding this central area is a bluer, more diffuse region, hinting at ongoing star formation. There's some subtle evidence of what may be spiral arm structures or tidal features, although the resolution limits a clear definition. Faint, extended blue patches are distributed around the galaxy, possibly representing areas of localized star formation. The overall morphology doesn't obviously align with a simple elliptical or spiral classification, which may denote a galaxy undergoing some interaction, potentially a minor merger event based on its slightly disturbed appearance. The color distribution suggests varying stellar populations and possibly differential dust extinction across the galaxy.
