The galaxy appears as a moderately inclined, disk-shaped system. Its overall color suggests a mixture of stellar populations. The central region is a brighter, more condensed zone with a bluer hue, indicative of ongoing or recent star formation activity. The outer disk presents a less defined structure, with fainter, somewhat redder tones that suggest the presence of older stellar populations. The morphology is generally smooth with some features that could be described as minor disturbances and/or merger activity, though no prominent tidal tails or dramatic asymmetries are evident. The galaxy's elongated shape is consistent with a late-type spiral or lenticular classification.
