The galaxy presents a relatively smooth, though slightly irregular, overall morphology. Its shape is somewhere between round and elongated, possibly tending towards a mild cigar shape. There appears to be a dominant central bulge exhibiting a yellowish-white hue, suggesting an older stellar population. Fainter, bluer regions are visible extending outward from the central bulge, potentially indicative of ongoing or recent star formation within a disk-like structure. The galaxy exhibits some signs of disturbance, such as asymmetry in the outer regions. There is no prominent spiral structure directly visible, but the distribution of the bluer regions implies the presence of some disklike structure. No significant tidal tails or obvious signs of an ongoing major merger are observed, though there is a suggestion of minor interaction. The estimated size appears moderate in scale.
